June 11, 2026
We prove a distributional convergence result for a multidimensional version of symmetric cooperative motion which was introduced and studied in one dimension in [1], [2]. Our approach relies on framing the associated recursive distributional equation as a discretization of the porous medium equation. A major challenge is to analyze the behaviour of finite difference schemes which approximate weak solutions of the porous medium equation with unbounded initial data. In overcoming this difficulty, we perform a detailed analysis of the probability mass function of symmetric cooperative motion, in which we introduce several new comparison arguments for the discrete process. Consequently, along the way, we establish a novel multidimensional convergence result for a finite difference scheme approximating the ZKB/Barenblatt solution of the porous medium equation, which is of independent interest.
We consider a multidimensional generalization of the process known as symmetric cooperative motion, which was considered in [1], [2]. Our process takes place in the lattice \(\mathbb{Z}^d\), where the neighbours of a point \(k\in \mathbb{Z}^d\) are the points \(k\pm e_i\) for \(i = 1, \ldots, d\), where \(\{e_{1},\dots,e_{d}\}\) is the standard basis of \(\mathbb{R}^{d}\).
For an integer \(m \geq 1\), a \(\mathop{\mathrm{CM}}(m,d)\)-cooperative motion started from \(0\in \mathbb{Z}^{d}\) is a \(\mathbb{Z}^d\)-valued stochastic process \((X^{n}, n \geq 0)\) defined as follows. Let \((E^{n}, n\geq 0)\) be IID with \({\mathbf{P}}\left\{E^1=\pm e_{i}\right\}=\frac{1}{2d}\) for all \(i\in \left\{1, \ldots, d\right\}=:[d]\). Starting from \(X^{0}=0\), we let \[\label{eq:defining95equation} X^{n+1}=\begin{cases} X^{n}+E^{n}&\text{if X^{n}=X^{n,1}=X^{n,2}=\ldots=X^{n,m}}\\ X^{n}&\text{otherwise}, \end{cases}\tag{1}\] where \(X^{n,1},\ldots X^{n,m}\) are \(m\) independent copies of \(X^n\).
As in [1], [2], one way to realize \(\mathop{\mathrm{CM}}(m,d)\)-cooperative motion is using a tree-indexed random process. Let \(\mathcal{T}\) be the complete rooted \((m+1)\)-ary tree, with root labeled \(\emptyset\) and node \(v\) having children \((vi: 1\leq i\leq m+1)\). Let \(\mathcal{T}_{n}\) denote the subtree of \(\mathcal{T}\) containing nodes at distance at most \(n\) from the root, and let \(\mathcal{L}_{n}\) denote the leaves of \(\mathcal{T}_{n}\).
For each \(n\in \mathbb{N}\), we let \(E^{n}=(E_v: v\in \mathcal{T}_{n}\setminus \mathcal{L}_{n})\) be as above. For \(v\in \mathcal{L}_{n}\), let \(\Sigma^{n}_{v}=0\in \mathbb{Z}^{d}\). For \(v\in \mathcal{T}_{n}\setminus \mathcal{L}_{n}\), we recursively define \[\Sigma^{n}_{v}:=\begin{cases}\Sigma^{n}_{v1}+E_{v}&\text{if \Sigma^{n}_{v1}=\Sigma^{n}_{v2}=\ldots=\Sigma^{n}_{v(m+1)}}\\ \Sigma^{n}_{v1}&\text{otherwise.} \end{cases}\] This recursion leads to an “output value” \(\Sigma^{n}_{\emptyset}\) at the root, which has the same distribution as \(X^{n}\). As described in [1], this model has natural connections to the random hierarchical lattice introduced by Hambly and Jordan [3]. In the case when \(m\) is positive and non-integer, one can still define a \(\mathop{\mathrm{CM}}(m,d)\)-distributed process, using a recursive distributional equation (RDE) (i.e. a process whose probability mass function defined by 4 satisfies 6 ). Moreover, by translating the process, one can also consider a \(\mathop{\mathrm{CM}}(m,d)\)-cooperative motion started at \(x\in \mathbb{Z}^{d}\).
The main result (and primary motivation) of this paper is the following distributional convergence result for a \(\mathop{\mathrm{CM}}(m,d)\)-distributed process in dimension \(d>1\).
Theorem 1. Let \(d>1\), \(m\geq 1\), and \((X^{n}, n \geq 0)\) be \(\mathop{\mathrm{CM}}(m,d)\)-distributed started from \(x\in \mathbb{Z}^{d}\). There exists an \(\mathbb{R}^{d}\)-valued random variable \(B\), whose density with respect to Lebesgue measure is given by \(\bar{u}(\cdot,1)\) as defined in 2 , such that \[\frac{X^{n}}{n^{1/(dm+2)}} \xrightarrow[n\to\infty]{d} B.\]
Observe that it is enough for us to prove Theorem 1 in the case when \(x=0\), since starting at an arbitrary \(x\in \mathbb{Z}^{d}\) does not affect the limiting distribution.
The function \(\bar{u}\) is defined by \[\label{e46Bdef} \bar{u}(x,t):=t^{-d\beta}(C-\gamma|x|^{2}t^{-2\beta})_{+}^{\frac{1}{m}},\tag{2}\] where \[\label{d46constants} \beta:=\frac{1}{dm+2}, \qquad \gamma:=\frac{d m \beta}{m+1},\tag{3}\] and \(C\) is a constant such that \(\int \bar{u}(x, t)\, dx=1\) for all \(t>0\). This function is known as the ZKB/Barenblatt solution [4], [5] (with mass \(1\)) of the porous medium equation (PME), which we will soon introduce. In the case where \(d=1\) and \(m=1\), the first and third author (with collaborators) proved this result in [1] for a generic initial distribution \(\mu\) (i.e. not necessarily started at a single point). In a subsequent work [2], in the case where \(d=1\) and \(m>0\) is arbitrary, the first and fourth author proved this result (with a collaborator) also for a generic initial distribution \(\mu\). In all of the prior cases, the limiting random variable in those results agrees with \(B\) as in Theorem 1. It is for this reason that Theorem 1 and all subsequent results of this paper are stated for \(d>1\). We expect that our proof technique could be adapted to the case \(d=1\), with suitable modifications, but we did not pursue this since the case \(d=1\) was already covered by the existing literature.
Our approach is to study the probability mass function of \(X^{n}\). For \(k=(k_{1}, \ldots, k_{d})\in \mathbb{Z}^{d}\) and \(n \in {\mathbb{N}}_{0} := {\mathbb{N}}\cup \{0\}\), let \[\label{e46pdef} p(k,n) := {\mathbf{P}}\left\{X^{n}=k\right\}.\tag{4}\]
As we will see in the sequel, \(p(k,n)\) satisfies an RDE which will tie the process to solutions of the PME. Our approach crucially relies on various properties of \(p(k,n)\), which require substantial new ideas to establish. This denotes the second major contribution of the current work. To state this contribution, we require one additional definition: for \(q: \mathbb{Z}^d \to \mathbb{R}\), we define the total variation of \(q\) on a set \(D \subset \mathbb{Z}^{d}\) as \[\label{e46dtv} [q]_{\mathop{\mathrm{TV}}(D)} := \frac{1}{2}\sum_{\{u,v\in D:\, u\sim v\}} |q(v)-q(u)|.\tag{5}\]
Theorem 2. Let \(d>1\), \(m\geq 1\) and \((X^{n}, n \geq 0)\) be \(\mathop{\mathrm{CM}}(m,d)\)-distributed started from 0. Let \(p(\cdot, n)\) be the PMF of \(X^{n}\) (as in 4 ). There exists \(C = C(d,m) > 0\) such that,
(i) For all \(k \in \mathbb{Z}^{d}\) and \(n \in {\mathbb{N}}\), \(p(k,n) \leq Cn^{-d\beta},\)
(ii) For all \(r > 0\) and \(n \in {\mathbb{N}}\), \(\sum_{k\in \mathbb{Z}^{d}\cap B_{rn^{\beta}}^{c}}p(k,n) \leq C \exp(-r/C)\),
(iii) For all \(r>0\) and \(n \in {\mathbb{N}}\), \([p(\cdot,n)]_{\mathop{\mathrm{TV}}(B_{rn^{\beta}}\cap\mathbb{Z}^{d})} \leq C r^{d-1}n^{-\beta},\)
where \(B_{rn^{\beta}}\) denotes the ball of radius \(rn^{\beta}\) in \(\mathbb{R}^{d}\), \(B_{rn^{\beta}}^{c}\) denotes its complement, and the discrete total variation \([\cdot]_{\mathop{\mathrm{TV}}(B_{rn^{\beta}}\cap\mathbb{Z}^{d})}\) is defined in 5 .
Properties (i)-(iii) are discrete versions of properties satisfied by the ZKB/Barenblatt solution \(\overline{u}\), which can be observed by direct inspection. Indeed, it is easy to see that \(\bar{u}(\cdot,t) \le ct^{-d\beta}\), \(\overline{u}(\cdot, t)\) is supported in a ball of radius \(ct^{\beta}\), and by a short calculation, for all \(r\leq C\) it holds that \([\overline{u}]_{\mathop{\mathrm{TV}}(B_{rt^{\beta}})}\sim \int_{B_{rt^{\beta}}}|\nabla_{x}\overline{u}(x,t)|\, dx\leq Cr^{d-1}t^{-\beta}\). Respectively, property (i) says that \(p\) shares the same decay in time, property (ii) conveys that most of the mass of \(p(\cdot, n)\) is concentrated in a ball of radius \(n^{\beta}\), and property (iii) obtains a similar bound on the discrete total variation of \(p(\cdot, n)\).
In the next subsection, we describe the RDE satisfied by \(p(k,n)\), and then frame the analysis of that RDE in the context of convergence of a finite difference scheme.
As a consequence of the definition of the process in 1 , it is easy to verify that the following relation holds: \[\label{e46pscheme} \begin{align} p(k,n+1) &=p(k,n)(1-p(k,n)^{m})+\frac{1}{2d}\sum_{\ell\sim k} p(\ell,n)^{m+1}\\ &=p(k,n)+\frac{1}{2d}\sum_{i=1}^{d} \left[p(k+e_{i},n)^{m+1}-2p(k,n)^{m+1}+p(k-e_{i},n)^{m+1}\right]\\ &=p(k,n)+\frac{1}{2d}\sum_{i=1}^d \sum_{\zeta \in \{-1, 1\}} \left[p(k+\zeta e_{i},n)^{m+1}-p(k,n)^{m+1}\right]. \end{align}\tag{6}\]
The above recurrence looks like the discretization of a PDE “at scale 1”. Throughout the paper, we will refer to recursive relations as schemes (short for finite difference schemes which are considered in numerical analysis). In order to connect 6 with a PDE, we introduce discrete meshes in time and space. For \(N\in {\mathbb{N}}\), we define \[\begin{align} \Delta_t= \Delta_t(N) := N^{-1} = \text{time mesh} \quad\text{and}\quad \Delta_x= \Delta_x(N) := N^{-1/(dm+2)} = \text{space mesh} \end{align}\] These parameters satisfy the relation \(\Delta_t= (\Delta_x)^{dm+2}\), which, as we will soon argue, is a natural scaling relation for the problem which keeps the associated PDE scale-invariant. We now define \(u_{N}: \mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t\to \mathbb{R}\) by \[\label{e46UNdef} u_{N}(k\Delta_x, n\Delta_t):= \frac{1}{(\Delta_x)^{d}}{\mathbf{P}}\left\{X^{n}=k\right\} = \frac{1}{(\Delta_x)^{d}}p(k,n).\tag{7}\] Using the relation \(\Delta_t= (\Delta_x)^{dm+2}\), we may rewrite 6 as \[\begin{align} \label{e46longscheme} & \frac{u_{N}(k\Delta_x, (n+1)\Delta_t)-u_{N}(k\Delta_x, n\Delta_t)}{\Delta_t}\notag\\ & = \frac{1}{2d (\Delta_x)^2 } \sum_{\ell \sim k} (u_N(\ell \Delta_x,n\Delta_t)^{m+1}-u_N(k \Delta_x,n\Delta_t)^{m+1})\notag\\ & =\frac{1}{2d}\sum_{i=1}^{d}\frac{u_{N}(k\Delta_x+e_{i}\Delta_x,n\Delta_t)^{m+1}-2u_{N}(k\Delta_x,n\Delta_t)^{m+1}+u_{N}(k\Delta_x-e_{i}\Delta_x,n\Delta_t)^{m+1}}{(\Delta_x)^{2}}. \end{align}\tag{8}\] This is a finite difference scheme which, formally, approximates the partial differential equation \[\label{e46genpm} u_{t}=\frac{1}{2d}\Delta(u^{m+1}),\tag{9}\] which is known as the porous medium equation (PME). The PME is a well-studied nonlinear PDE which has a rich theory of analysis (see for example [6] for a broad overview of the PME). The ZKB/Barenblatt solution \(\bar{u}\) introduced in 2 is a type of “weak solution” of the PME, with initial condition the Dirac delta measure \(\delta\), where the notion of solution and initial condition will be made precise in Section 6.2.
In light of the relation 7 , Theorem 1 follows easily if we can prove that \[\label{e46punchline} \lim_{N\to\infty} u_{N}(\cdot ,1)=\bar{u}(\cdot ,1)\quad\text{in L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}).}\tag{10}\] This statement is a convergence result for a scheme 8 of the porous medium equation 9 . The typical perspective is to start from an initial condition \(u_{0}:\mathbb{R}^{d}\rightarrow \mathbb{R}\), and use this to define \(u_{N}(\cdot, 0)\) by a suitable discretization (see, for example, 18 , below). By generating \(u_{N}\) at later times using the scheme, the goal is to show that \(u_{N}\) converges to the solution of the PME with initial condition \(u_{0}\). Thus, if we had at our disposal a convergence result for \((u_{N})_{N\geq 1}\), for which the discretization of the initial condition was given exactly by \[u_{N}(k\Delta_x, 0)=\frac{1}{(\Delta_x)^{d}}p(k,0)=\begin{cases}\frac{1}{(\Delta_x)^{d}}&\text{if k=0},\\ 0&\text{otherwise,} \end{cases}\] then 10 would be automatic.
As in [1], [2], [7], the introduction of the finite difference schemes perspective has been fruitful for proving distributional convergence results for cooperative motions. The approach has further been used by Morfe [8] and Chen, Duquesne, and Shi [9] in analyzing a variety of discrete random models, including the resistance of the series-parallel graph. Similar to the challenges in [1], [2], [7], the key issue is that the only initial condition \(u_{0}\) for which a suitable discretization yields the above initial condition for \(u_{N}\) is for \(u_{0}=\delta\), the Dirac delta, the probability distribution which assigns mass 1 to the point 0 in \(\mathbb{R}^{d}\). Convergence results for finite difference schemes approximating PME with initial conditions \(u_{0}\in L^{\infty}(\mathbb{R}^{d})\) have been well-studied in the literature (see for example [10] which holds for inviscid and viscous conservation laws, for which the PME is a special case). However, to our knowledge, there are limited convergence results for finite difference schemes approximating weak solutions to the PME with unbounded, measure-valued initial conditions in dimensions greater than 1.
In the case when \(d=1\), it was possible to circumvent this lack of convergence results in two different ways. In [1], the authors used a convergence result of Evje and Karlsen [11] for finite difference schemes approximating entropy solutions of the PME with carefully chosen, bounded, initial conditions. By a coupling argument, the authors were then able to establish the statement of Theorem 1 in the case when \(d=1\) and \(m=1\). In [2], the authors proved distributional convergence by considering the cumulative distribution function (CDF) of the process, which, in one dimension, satisfies an RDE which approximates another nonlinear PDE known as the the parabolic \(p\)-Laplace equation. By considering the CDF, one essentially gains an additional level of regularity (and access to a more robust theory of convergence results for finite difference schemes, such as the one established in the work of Barles and Souganidis [12]). Using these convergence results for finite difference schemes with suitable initial conditions, combined with monotone coupling arguments, the authors of [2] established the distributional convergence in Theorem 1 for all \(m>0\) and \(d=1\).
In dimensions larger than 1, neither of these approaches seemed feasible, because the coupling arguments in both of the prior works relied heavily on the one-dimensional nature of the process. Consequently, due to the lack of convergence results for finite difference schemes approximating the PME with unbounded, measure-valued initial data, we overcame this by proving our own. We prove that 10 holds in Theorem 55, which is the third major contribution of our work. Our proof relies heavily on the properties of the probability mass function \(p\) established in Theorem 2; this allows us to perform a compactness argument for a suitable family of approximations to extract a convergent limit with the correct initial condition. For the approximations, we rely on the priorly mentioned convergence results of Karlsen and Risebro [10] for finite difference schemes approximating entropy solutions of the PME with \(L^{\infty}\) initial data.
While writing this paper, we became aware of a convergence result recently proven by Di Francesco and Matthes [13] for a discrete scheme (which is not a finite difference scheme) approximating distributional solutions to the PME in one dimension with initial condition a probability measure with density \(u_{0}\in L^{1}(\mathbb{R})\). More generally, the authors of [13] were interested in analyzing the evolution of a discrete interacting particle system, which is another very interesting way in which the PME has arisen in probabilistic settings. Nevertheless, their result and their methods (which are specific to \(d=1\) and the particular discrete scheme they work with) do not apply to our setting. In general, it seems that there is a fundamental challenge to proving convergence results for schemes approximating the PME with unbounded initial data, which requires new ideas to overcome.
The prior discussion highlights another challenge in this setting, which is that the Barenblatt solution can be interpreted as many different types of “weak solutions” of the PME. It is both a nonnegative entropy solution and a distributional solution (see Section 6.2 for a detailed discussion). In this paper, we navigate between these two notions, which adds an additional layer of technical care which must be taken into account in our analysis.
As priorly mentioned, the proofs of Theorem 1 and of Theorem 55 rely crucially on the properties of the probability mass function \(p=p(k,n)\) of the \(\mathop{\mathrm{CM}}(m,d)\)-distributed process \((X_{n}, n\geq 0)\). In this subsection, we describe some of the main ideas in the proof of Theorem 2. In light of the discussion following the statement of Theorem 2, the three properties of \(p\) which are established are analogous to three properties observed by the Barenblatt solution \(\bar{u}\).
The first property, which is a type of \(L^{\infty}\)-estimate for solutions of the PME, is traditionally proven using the celebrated Aronson-Benilan estimate on the pressure [6], [14]. While there have been some works examining a discrete-in-space, continuous-in-time version of the Aronson-Benilan estimate on locally finite graphs [15], as well as the aforementioned work [13] for an interacting particle system when \(d=1\), we do not establish a discrete version of the Aronson-Benilan estimate in this work. However, our approach does bear some similarities to theirs.
We begin by restricting our analysis to solutions of the finite difference scheme 6 which are radially symmetric in space in an \(\ell^{1}\) sense (we refer to these functions as volcanic functions in space). Under certain assumptions on the \(\ell^{\infty}\)-norm of the initial condition, the scheme 6 is monotone, in the sense that solutions of the scheme with ordered initial data remain ordered at all future times. Generally speaking, the theory of convergence for monotone finite difference schemes is quite robust, because it allows one to access comparison methods. We establish several properties for solutions of finite difference schemes with volcanic initial data, which remain volcanic in space for all times (we hereby refer to these functions simply as volcanic).
Upon restricting to volcanic functions, we give a new interpretation of how a solution of the finite difference scheme can be seen as a type of lazy random walk. This allows us to prove a general estimate, Theorem 12 below, which says that if a volcanic solution of the finite difference scheme is bounded from below in a certain scaled neighborhood of the origin, then it must be bounded from above by a comparable bound in the entire space. The rough idea is to use the local lower bound as a lower bound on the “jump probability” of associated lazy random walk. In the theory of PDEs, this would be like having a lower bound on the ellipticity of a differential operator. This (local) lower bound can then be upgraded to a uniform upper bound, which plays a similar role to that played by Aronson-Benilan estimates on the pressure.
In order to establish the desired local lower bound on a volcanic solution, we develop a comparison theory between solutions of the scheme and so-called approximate solutions of the scheme. In particular, we use a discretization of the Barenblatt solution as an approximate solution, and based on the comparison theory we establish, we prove the local lower bound on a volcanic solution. The final challenge is that the probability mass function \(p\) is not actually volcanic for all times. Thus, we require one additional level of comparison to relate \(p\) to a volcanic solution. This completes the proof sketch of Theorem 2(i).
The proofs of Theorem 2(ii), (iii) follow relatively easily from Theorem 2(i). To prove Theorem 2(ii), we use a concentration inequality known as Freedman’s inequality (Theorem 31). In applying Freedman’s inequality, the bound in Theorem 2(i) is crucial as it allows us to control the conditional variance of projections of the original process. The proof of Theorem 2(iii) also follows relatively easily from the upper bound in Theorem 2(i); we just need to introduce a suitable approximation to compare the true solution \(p\) of the finite difference scheme to a volcanic one.
The structure of the remainder of the paper is as follows. In Section 2, we begin by introducing some notation, terminology, and basic properties used throughout the paper. In Section 3, we present the proof of Theorem 12, which gives another interpretation of volcanic solutions of the finite difference scheme in terms of a lazy random walk. In Section 4, we complete the proof of Theorem 2(i). In Section 5, we prove the remaining parts of Theorem 2. Finally, in Section 6, we prove both Theorem 55 and the remaining parts of Theorem 1; we use the properties of \(p\) obtained from Theorem 2 to perform the compactness argument for suitable approximations. In the Appendix, we provide the proofs of some technical estimates which are used in Section 3.
We use the notation \([d]:=\left\{1,2, \ldots, d\right\}\). We let \({\mathbb{N}}\) be the positive integers and define \({\mathbb{N}}_{0}:={\mathbb{N}}\cup \{0\}\). For \(T > 0\), we let \(Q_{T} := \mathbb{R}^{d} \times (0,T)\). We use \(C\) and \(c\) to denote positive constants which depend only on \(d\) and \(m\), and which may change from line to line. We use \(x, y, z\) for points in \(\mathbb{R}^d\), and \(k, \ell\) for points in \(\mathbb{Z}^{d}\). If \(k,\ell\in \mathbb{Z}^{d}\) are neighbors, i.e. \(k-\ell=\pm e_{i}\) for some \(i\in [d]\), then we write \(k\sim \ell\). For \(x\in\mathbb{R}^d\), we denote the Euclidean norm of the point using single vertical bars, \(|x| = (x_1^2 + \cdots + x_d^2)^{1/2}\), while \(|x|_1 = \sum_{i=1}^d |x_i|\) refers to the \(1\)-norm of the point.
For measurable functions \(v: U \to \mathbb{R}\) where \(U \subset \mathbb{R}^{d}\) or \(U \subset\mathbb{R}^{d}\times[0,\infty)\), and \(p\in (0, \infty)\), we denote the \(L^p\)-norm of \(v\) by \(\|v\|_{L^{p}(U)}=(\int_U |v (x)|^p\, dx)^{1/p}\). Similarly, for \(q: \mathbb{Z}^d \to \mathbb{R}\), we write \(\|q\|_{L^p(\mathbb{Z}^{d})}=(\sum_{k \in \mathbb{Z}^d} |v(k)|^p)^{1/p}\). We write \(L^{\infty}(\mathbb{R}^{d})\) for the space of essentially bounded functions on \(\mathbb{R}^{d}\), and \(L^{\infty}(\mathbb{Z}^{d})\) (respectively, \(L^{\infty}(\mathbb{Z}^{d}\Delta_x)\)) for the set of bounded functions on the discrete lattice \(\mathbb{Z}^{d}\) (respectively, \(\mathbb{Z}^{d}\Delta_x\)).
We next extend the definition of total variation from lattice functions to more general functions, and introduce the bounded variation norm. If \(U \subset \mathbb{R}^d\) open and \(v \in L^1(U)\), then the total variation of \(v\) is given by \[\label{eq:tv95cont} [v]_{\mathop{\mathrm{TV}}(U)} := \sup\left\{\int_{U} v \mathop{\mathrm{div}}(w)\,dx : w \in C^{\infty}_{c}(U;\mathbb{R}^{d}), |w(\cdot)| \leq 1\right\},\tag{11}\] where \(C^{\infty}_{c}(U;\mathbb{R}^{d})\) is the set of smooth functions with compact support from \(U\) to \(\mathbb{R}^{d}\). We define the bounded variation norm of \(v\) by \(\|v\|_{\mathop{\mathrm{BV}}(U)} = \|v\|_{L^{1}(U)} + [v]_{\mathop{\mathrm{TV}}(U)}\), and we denote the Banach space \(\mathop{\mathrm{BV}}(U) := \{v : U \to \mathbb{R}: \|v\|_{\mathop{\mathrm{BV}}(U)} < \infty\}\).
For \(\Lambda>0\) and \(U \subset \mathbb{R}^d\), we let \[\mathcal{B}_{\Lambda}^+(U)= \{u:U \to [0,\Lambda]\}.\]
Lastly, we introduce some additional notation regarding sets and extensions of functions from \(\mathbb{Z}^{d}\) to all of \(\mathbb{R}^{d}\). For \(N\in \mathbb{N}\), we define \[\square_{N} := \left[-\frac{\Delta_x}{2},\frac{\Delta_x}{2}\right)^{d}= \left[-\frac{\Delta_x(N)}{2},\frac{\Delta_x(N)}{2}\right)^{d} = \left[-\frac{N^{-1/(dm+2)}}{2},\frac{N^{-1/(dm+2)}}{2}\right)^{d},\] and note that \(|\square_N|:= \int \boldsymbol{1}_{\square_N}(x)dx = (\Delta_x)^d\). For every \(k\in \mathbb{Z}^d\), we let \[\square_{N}(k\Delta_x) = \square_{N} + k\Delta_x.\] We say that \(w_{N}: \mathbb{R}^{d} \to \mathbb{R}\) is \((\mathbb{Z}^{d}\Delta_x)\)-piecewise constant if \[w_{N}(x) = w_{N}(k\Delta_x) \text{ for all } x \in \square_{N}(k\Delta_x).\] Likewise, we say that \(w_{N}: \mathbb{R}^{d} \times [0,\infty) \to \mathbb{R}\) is \((\mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t)\)-piecewise constant if \[v_{N}(x,t) = v_{N}(k\Delta_x,n\Delta_t) \text{ for all } (x,t) \in \square_{N}(k\Delta_x)\times [n\Delta_t,(n+1)\Delta_t).\]
Given \(A: \mathbb{R}\rightarrow \mathbb{R}\), define \(\mathcal{S}=\mathcal{S}[A]: L^{\infty}(\mathbb{Z}^{d}) \to L^{\infty}(\mathbb{Z}^{d})\) by \[\label{d46Sdef} \mathcal{S}q(k) := q(k) +\frac{1}{2d}\sum_{\ell\sim k} \left[A(q(\ell)) - A(q(k))\right],\quad\text{where q\in L^{\infty}(\mathbb{Z}^{d}).}\tag{12}\] We say a sequence of functions \(q=(q_{n})_{n \ge n_{0}}\) is a solution of scheme \(\mathcal{S}\) on \([n_{0}, \infty)\) with initial condition \(f: \mathbb{Z}^{d}\rightarrow \mathbb{R}\) if \[\label{e46operator} \begin{cases} q_{n+1} = \mathcal{S}q_n=q_{n}(k) +\frac{1}{2d}\sum_{\ell\sim k} \left[A(q_{n}(\ell)) - A(q_{n}(k))\right]&\text{for n\geq n_{0},}\\ q_{n_{0}}=f. \end{cases}\tag{13}\]
Throughout the paper, we will frequently consider functions \(\tilde{p}=(\tilde{p}_{n}(k))_{n\geq n_{0}}\) with initial condition \(f\) solving \[\label{timeevol} \begin{cases} \tilde{p}_{n+1}(k) = \tilde{p}_{n}(k) + \frac{1}{2d} \sum_{\ell \sim k} \left[A(\tilde{p}_{n}(\ell)) - A(\tilde{p}_{n}(k))\right]&\text{with A(u) = u^{m+1}, for n\geq n_{0}},\\ \tilde{p}_{n_{0}}=f. &{} \end{cases}\tag{14}\] Instead of referring to \(\tilde{p}\) as the solution of \(\mathcal{S}[A]\) with \(A(u)=u^{m+1}\), we simply refer to \(\tilde{p}\) as the solution of the discrete PME on \([n_{0}, \infty)\) with initial condition \(f\).
For the function \(p\) defined in 4 and appearing in 6 , setting \(p_n(k) = p(k, n)\), we see that \(p\) is a solution of the discrete PME 14 on \([0, \infty)\) with initial condition \(\boldsymbol{1}_{0}\).
We next define a notion of monotonicity of schemes. Fix a collection of functions \(\mathcal{C}\subset L^\infty(\mathbb{Z}^d)\) and a mapping \(\mathcal{S}:\mathcal{C}\to L^\infty(\mathbb{Z}^d)\). We say \(\mathcal{S}\) is monotone on \(\mathcal{C}\) if \(\mathcal{S}(\mathcal{C})\subset \mathcal{C}\), and \(\mathcal{S}q \le \mathcal{S}\tilde{q}\) pointwise whenever \(q,\tilde{q} \in \mathcal{C}\) are functions such that \(q \le \tilde{q}\) pointwise. We say \(\mathcal{S}\) is locally monotone on \(\mathcal{C}\) if \({\mathcal{S}}(\mathcal{C})\subset \mathcal{C}\), and for any \(k \in \mathbb{Z}^d\), \((\mathcal{S}q)(k) \le (\mathcal{S}\tilde{q})(k)\) whenever \(q,\tilde{q} \in \mathcal{C}\) are such that \(q(\ell)\le \tilde{q}(\ell)\) for all \(\ell \in \mathbb{Z}^d\) with \(|\ell-k|_{1}\leq 1\). Note that local monotonicity implies monotonicity, since if \(q \le \tilde{q}\) pointwise then in particular \(q(\ell)\le \tilde{q}(\ell)\) for all \(\ell\) with \(|\ell-k|_{1}\leq 1\), for any \(k \in \mathbb{Z}^d\).
Lemma 3. Fix a differentiable function \(A:\mathbb{R}\to\mathbb{R}\) with \(A'(\cdot) \in [0,1]\) and define an operator \(\mathcal{S}=\mathcal{S}[A]:L^\infty(\mathbb{Z}^d)\to L^\infty(\mathbb{Z}^d)\) by 12 . Then \(\mathcal{S}\) is locally monotone (and consequently monotone) on \(L^\infty(\mathbb{Z}^d)\), and for any non-negative \(q \in L^\infty(\mathbb{Z}^d)\), it holds that \(0 \le \mathcal{S}q \le \|q\|_{L^\infty(\mathbb{Z}^{d})}\).
Proof. Observe that \(A(u)\) and \(u-A(u)\) are nondecreasing functions in \(u\), since \(A'(\cdot) \in [0,1]\). Fix functions \(q, \tilde{q} \in L^{\infty}(\mathbb{Z}^d)\), and suppose \(k\in \mathbb{Z}^{d}\) is such that \(q(\ell)\leq q'(\ell)\) for all \(|\ell-k|_{1}\leq 1\). Then by the previous observation, \[\begin{align} \mathcal{S}q(k) &= q(k) + {1 \over 2d} \sum_{\ell\sim k} \left[A(q(\ell)) - A(q(k))\right] \\&= q(k) - A(q(k)) + {1 \over 2d} \sum_{\ell\sim k} A(q(\ell)) \\&\le q'(k) - A(q'(k))+ {1 \over 2d} \sum_{\ell\sim k} A(q'(\ell)). \\&=\mathcal{S}q'(k). \end{align}\] Since constants are solutions of the scheme \(\mathcal{S}\), it follows that \(0 \le \mathcal{S}q \le \|q\|_{L^\infty(\mathbb{Z}^{d})}\), which implies that \(\mathcal{S}q\in L^{\infty}(\mathbb{Z}^{d})\). Thus, \(\mathcal{S}\) is indeed locally monotone (and consequently monotone). ◻
For \(\Lambda > 0\), the same argument applied to the function class \(\mathcal{B}_{\Lambda}^+(\mathbb{Z}^d)\) gives the following result, whose proof is omitted.
Corollary 4. Fix a constant \(\Lambda>0\) and a function \(A:\mathbb{R}\to\mathbb{R}\) such that \(A'(u) \in [0,1]\) whenever \(u \in [0,\Lambda]\). Define an operator \(\mathcal{S}=\mathcal{S}[A]:L^\infty(\mathbb{Z}^d)\to L^\infty(\mathbb{Z}^d)\) by 12 . Then \(\mathcal{S}\) is locally monotone (and consequently monotone) on \(\mathcal{B}_{\Lambda}^+(\mathbb{Z}^{d})\).
The operator \(\mathcal{S}\) also has some desirable properties with respect to \(\|\cdot\|_{L^1(\mathbb{Z}^{d})}\).
Lemma 5. Assume that there exists \(\Lambda> 0\) such that \(\mathcal{S}=\mathcal{S}[A]\) is monotone on \(\mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\). Assume further that \(A: \mathbb{R}\rightarrow \mathbb{R}\) is such that \(A'(u) \in [0,1]\) for \(u \in [0,\Lambda]\). It follows that
(i) For all \(q \in L^1(\mathbb{Z}^{d}) \cap \mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\), \(\sum_{k\in \mathbb{Z}^{d}} \mathcal{S}q(k) = \sum_{k\in \mathbb{Z}^{d}} q(k)\),
(ii) For all \(q, q' \in L^1(\mathbb{Z}^{d}) \cap \mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\), \(\Vert \mathcal{S}q - \mathcal{S}q' \Vert_{L^1(\mathbb{Z}^d)} \le \Vert q - q' \Vert_{L^1(\mathbb{Z}^d)}\).
Proof. To prove (i), notice that since \(A'(u) \in [0,1]\) for all \(u \in [0,\Lambda]\), it follows that \(0 \leq A(q) \leq q\), where \(q\in L^{1}(\mathbb{Z}^{d})\). Hence, we can rearrange the sum, \[\begin{align} \sum_{k\in \mathbb{Z}^{d}} (\mathcal{S}q(k) - q(k)) &= {1 \over 2d} \sum_{i=1}^d \sum_{\zeta \in \{-1, 1\}} \left[\sum_{k\in \mathbb{Z}^{d}} A(q(k+ \zeta e_i)) - \sum_{k\in \mathbb{Z}^{d}} A(q(k))\right] \\&= {1 \over 2d} \sum_{i=1}^d \sum_{\zeta \in \{-1, 1\}} \left[\sum_{\ell\in \mathbb{Z}^{d}} A(q(\ell)) - \sum_{k\in \mathbb{Z}^{d}} A(q(k))\right] \\&= 0, \end{align}\] which is precisely the statement of (i). The inequality in (ii) is a consequence of [16]. ◻
In the case of the discrete PME, when \(A(u) = u^{m+1}\), we obtain the following.
Corollary 6. When \(A(u) = u^{m+1}\), the associated operator \(\mathcal{S}=\mathcal{S}[A]\) satisfies
(i) The scheme \(\mathcal{S}[A]\) is monotone on \(\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\).
(ii) For all \(q \in L^1(\mathbb{Z}^{d}) \cap \mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\), \(\sum_k\mathcal{S}q(k) = \sum_kq(k)\),
(iii) For all \(q, q' \in L^1(\mathbb{Z}^{d}) \cap \mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\), \(\Vert \mathcal{S}q - \mathcal{S}q' \Vert_{L^1(\mathbb{Z}^{d})} \le \Vert q - q' \Vert_{L^1(\mathbb{Z}^{d})}\).
Proof. By Corollary 4, we simply need to check that \(A'(u)\in [0,1]\) whenever \(u\in [0, \frac{1}{2}]\). By direct computation, \(A'(u) = (m+1)u^m\), and since \(m\geq 1\), it follows that \(A'(0)\leq A'(u)\leq A'(\frac{1}{2})\). In the case when \(m=1\), it is clear that \(0\leq A'(u)\leq 1\), which implies the claim. Moreover, it can be seen that \(A'(\frac{1}{2})\) is decreasing in \(m\ge 1\), since \[{d \over dm} (m+1)\frac{1}{2^{m}} = (1 - (m+1)\log 2)\frac{1}{2^{m}},\] which is strictly negative when \(m>1\). The second two claims follow by Lemma 5. ◻
Akin to the above, we can also consider the operator perspective on the scaled lattice \(\mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t\). Let \(\mathcal{S}_{N}: L^{\infty}(\mathbb{Z}^{d}\Delta_x) \to L^{\infty}(\mathbb{Z}^{d}\Delta_x)\) be defined by \[\label{e46SN} \mathcal{S}_{N}v(k\Delta_x)= v(k\Delta_x)+\frac{\Delta_t}{2d (\Delta_x)^2}\sum_{\ell \sim k}\left[A(v(\ell \Delta_x))-A(v(k\Delta_x))\right],\tag{15}\] where \(k, \ell\in \mathbb{Z}^{d}\). We may also identify \(\mathcal{S}_{N}\) with a scheme \(\mathcal{S}^{\Delta_x}_{N}: L^{\infty}(\mathbb{Z}^{d})\rightarrow L^{\infty}(\mathbb{Z}^{d})\), by using input functions of the form \(q(k):=v(\Delta_xk)\). By doing so, the notions of local monotonicity and monotonicity can naturally be extended to \(\mathcal{S}_{N}\). The finite difference scheme for \(u_{N}\), 8 , can then be written as \[\label{e46scheme} u_{N}(\cdot,(n+1)\Delta_t) = \mathcal{S}_{N}u_{N}(\cdot,n\Delta_t).\tag{16}\]
For initial conditions of \(u_{N}(\cdot, 0)\), we introduce two notions. Given a Radon measure \(\mu\) on \(\mathbb{R}^{d}\), we say that \(u_{N}\) is generated by \(\mathcal{S}_{N}\) with initial measure \(\mu\) if \(u_{N}\) is the unique \((\mathbb{Z}^{d}\Delta_x\times {\mathbb{N}_{0}}\Delta_t)\)-piecewise constant function satisfying 16 and \[\label{e46initmeas} u_{N}(k\Delta_x,0) = \frac{1}{|\square_{N}|}\mu(\square_{N}(k\Delta_x)).\tag{17}\] If there exists \(u_{0} \in L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\) such that \(d\mu=u_{0}\, dx\), then we say that \(u_{N}\) is generated by \(\mathcal{S}_{N}\) with initial condition \(u_{0}\); in other words, \[\label{e46initL1} u_{N}(k\Delta_x,0) = \frac{1}{|\square_{N}|}\int_{\square_{N}(k\Delta_x)}u_{0}(x)\,dx.\tag{18}\]
Remark 7. Let \(u_{N}: \mathbb{R}^{d} \times [0,\infty)\rightarrow \mathbb{R}\) be the \((\mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t)\)-piecewise constant function defined by \[u_{N}(k\Delta_x,n\Delta_t) := \frac{1}{|\square_{N}|} {\mathbf{P}}\left\{X^{n} = k\right\} = \frac{1}{(\Delta_x)^{d}}p(k,n).\] By rearranging the scheme 8 satisfied by \(u_{N}\), we see that \(u_{N}\) is generated by \(\mathcal{S}_{N}[A]\) with \(A(u) = u^{m+1}\). As for initial conditions, let \(\delta\) denote the probability measure on \(\mathbb{R}^{d}\) with \(\delta(\left\{0\right\})=1\) (we also refer to this as the Dirac \(\delta\)). Then \[\begin{align} u_{N}(k\Delta_x,0) = \frac{1}{|\square_{N}|} {\mathbf{P}}\left\{X^{0} = k\right\} = \frac{\delta(\square_{N}(k\Delta_x))}{|\square_{N}|}. \end{align}\] Hence, “\(u_{N}\) generated by \(\mathcal{S}_{N}[A]\) with \(A(u) = u^{m+1}\) and initial measure \(\delta\)” and “\(u_{N}\), the unique \((\mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t)\)-piecewise constant function satisfying eq. ¿eq:e46UNdef?” are two equivalent ways of defining the same function.
Analogous to Corollary 6, we next show that \(\mathcal{S}_{N}\) has desirable properties on a certain family. However, due to the additional parameter \(N\), we are able to allow for a more general family.
Lemma 8. Fix \(\Lambda> 0\). Suppose \(N\) is sufficiently large such that \[\label{e46cfl} N^{dm\beta} \geq 4(m+1)\Lambda^{m}.\qquad{(1)}\] Let \(\mathcal{S}_{N}=\mathcal{S}_N[A]\) be as defined in 15 with \(A(u)=u^{m+1}\). For \(n\in {\mathbb{N}}\), let \(\mathcal{S}_{N}^{n}\) be the \(n\)-fold composition of \(\mathcal{S}_{N}\). Then the following holds,
(i) The scheme \(\mathcal{S}_{N}\) is monotone on \(L^{\infty}(\Delta_x\mathbb{Z}^{d})\cap \mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\).
(ii) For \(w \in L^{\infty}(\Delta_x\mathbb{Z}^{d})\cap\mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\), for any \(n\geq 1\), \[\|\mathcal{S}_{N}^{n}w\|_{L^{\infty}(\Delta_x\mathbb{Z}^{d})}\leq \|w\|_{L^{\infty}(\Delta_x\mathbb{Z}^{d})}\] and thus \(\mathcal{S}_{N}^{n}\in L^{\infty}(\Delta_x\mathbb{Z}^{d})\cap\mathcal{B}_{\Lambda}^{+}(\mathbb{R}^{d})\).
(iii) For \(w, w' \in L^{1}(\mathbb{R}^{d}) \cap \mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\cap L^{\infty}(\Delta_x\mathbb{Z}^{d})\), \[\|\mathcal{S}_{N}^{n}w - \mathcal{S}_{N}^{n}w'\|_{L^{1}(\mathbb{R}^{d})} \leq \|w - w'\|_{L^{1}(\mathbb{R}^{d})}.\]
Proof. To show (i), we consider \(\tilde{A}(u):=\frac{\Delta_t}{(\Delta_x)^{2}}A(u)\). Then 15 can be rewritten as \[\mathcal{S}_{N}v(k\Delta_x)=v(k\Delta_x)+\frac{1}{2d}\sum_{k\sim \ell}\left[\tilde{A}(v(\ell \Delta_x))-\tilde{A}(v(k\Delta_x))\right].\] Using the identification with \(\mathcal{S}_{N}^{\Delta_x}: L^{\infty}(\mathbb{Z}^{d})\rightarrow L^{\infty}(\mathbb{Z}^{d})\), we now appeal to Lemma 3. For this, it is enough to check that \(\tilde{A}'(u)\in [0,1]\) for all \(u\in [0, \Lambda]\). Noting that \(\tilde{A}'(u)=\frac{\Delta_t}{(\Delta_x)^{2}}(m+1)u^{m}\), and recalling that \(\frac{\Delta_t}{(\Delta_x)^2} = \frac{N^{-1}}{N^{-2/(dm+2)}} = N^{-dm\beta}\), this implies that \[\tilde{A}'(u)=N^{-dm\beta}(m+1)u^{m}.\] For \(u\in [0, \Lambda]\), it follows by hypothesis ?? that \(\tilde{A}'(u)\in [0,1]\). Hence, an application of Lemma 3 yields (i).
To see (ii), note that the second conclusion of Lemma 3 gives that \(0 \leq \mathcal{S}_{N}w\leq \|w\|_{L^{\infty}(\mathbb{R}^{d})} \leq \Lambda\), meaning \(\mathcal{S}_{N}w \in \mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\cap L^{\infty}(\Delta_x\mathbb{Z}^{d})\). By iteration, we have (ii).
To prove property (iii), we remark that for a \(\Delta_x\mathbb{Z}^{d}\)-piecewise constant function \(w\), \(\int_{\mathbb{R}^{d}} |w(x)|\, dx=\sum_{k\in \mathbb{Z}^{d}} (\Delta_x)^{d}|w(k\Delta_x)|=(\Delta_x)^{d}|w(\cdot \Delta_x)|_{1}\). Therefore, the case \(n=1\) follows directly from Lemma 5. By setting \(w'_{N} \equiv 0\), we have \(\|\mathcal{S}_{N}w_{N}\|_{L^{1}(\mathbb{R}^{d})} \leq \|w_{N}\|_{L^{1}(\mathbb{R}^{d})}\). This fact, along with property (ii) says that \(\mathcal{S}_{N}w_{N} \in L^{1}(\mathbb{R}^{d}) \cap \mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\cap L^{\infty}(\Delta_x\mathbb{Z}^{d})\) whenever \(w_{N} \in L^{1}(\mathbb{R}^{d}) \cap \mathcal{B}^{+}_{\Lambda}(\mathbb{R}^{d})\cap L^{\infty}(\Delta_x\mathbb{Z}^{d})\). Hence, we can conclude property (iii) for all \(n\) by iteratively applying Lemma 2.4. ◻
We say that a function \(q: \mathbb{Z}^d \to \mathbb{R}\) is nondecreasing towards the origin if, for every two neighbours \(k\sim \ell\) in \(\mathbb{Z}^d\) with \(|k|_{1} > |\ell|_{1}\), we always have \(q(k) \le q(\ell)\). That is, if we take one step toward the origin on \(\mathbb{Z}^d\), in the \(\ell^{1}\)-sense, the function does not decrease.
We note that this does not imply that \(q(k) \le q(\ell)\) for any two points \(k, \ell\) with \(|k|_{1} > |\ell|_{1}\). For example, in two dimensions, we can define \[q(k) = \begin{cases}1&\text{ if } k_1 = 0 \text{ or } k_2 = 0\\0&\text{ otherwise.}\end{cases}\] This is nondecreasing toward the origin. However, \(|(0,3)|_{1}=3> |(1,1)|_{1}=2\), while \(q((0,3))=1> q((1,1))=0\).
We say that a function \(q: \mathbb{Z}^d \to \mathbb{R}\) is symmetric if the value of \(q\) remains the same when the input arguments are reflected in any coordinate plane, and when any pair of coordinates is transposed. That is, for any permutation \(\pi \in S_d\) and \(\varepsilon_1, \ldots, \varepsilon_d \in \{\pm1\}\), \[\label{e46symmdef} q(\varepsilon_1 k_{\pi(1)}, \ldots, \varepsilon_d k_{\pi(d)}) = q(k_1, \ldots, k_d).\tag{19}\]
If \(q\) is symmetric and nondecreasing toward the origin, we call \(q\) a volcanic function. For \(\Lambda>0\), we say that the scheme (14 ) is volcano-preserving on \(\mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\) if \(\mathcal{S}q\) is volcanic whenever \(q \in \mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\) is volcanic.
We now provide a sufficient condition on \(A\) to guarantee that \(\mathcal{S}\) is volcano-preserving.
Lemma 9. Fix \(\Lambda>0\) and let \(A: \mathbb{R}\rightarrow \mathbb{R}\) be such that \(0\leq A'(\cdot)\leq \frac{2}{3}\) on \([0,\Lambda]\). Then the scheme \[\mathcal{S}q(k) := q(k) +\frac{1}{2d}\sum_{\ell\sim k} \left[A(q(\ell)) - A(q(k))\right]\] defined by 12 is volcano-preserving on \(\mathcal{B}^{+}_{\Lambda}(\mathbb{Z}^{d})\).
Proof. Let \(q\) be a volcanic function. We now check that \(\mathcal{S}(q)\) is volcanic, under the hypotheses.
By the definition of \(\mathcal{S}\), if we compose \(q\) with some reflection or coordinate transposition, then \(\mathcal{S}q\) will undergo the same reflection or transposition, so \(\mathcal{S}q\) is symmetric.
Let \(k, \ell\) be neighbours with \(|k|_{1} > |\ell|_{1}\). The proof is complete if we can show \(\mathcal{S}q(k) \le \mathcal{S}q(\ell)\). By symmetry, we can assume without loss of generality that \(k\) and \(\ell\) differ in the first coordinate, and \(\ell_1 \ge 0\), so that the two points are \[\ell= (\ell_1, \ell_2, \ldots, \ell_d), \qquad k= (\ell_1 + 1, \ell_2, \ldots, \ell_d).\] We consider two cases.
Case 1. \(\ell_1 \ge 1\). We use the local monotonicity property of \(\mathcal{S}\). In this case, every coordinate \(\ell_i\) has the same sign as the corresponding coordinate \(k_i\). Let \(v\sim 0\) be a neighbour of the origin, and we will compare \(k+v\) and \(\ell+v\). If \(v = \pm e_i\) with \(i\neq 1\), then \(|\ell_{1}|<|k_{1}|\) and \(|\ell_{i}\pm1|=|k_{i}\pm1|\). If \(v=\pm e_{1}\), then since \(\ell_{1}\geq 1\), we still have \(|\ell_{1}\pm1|<|k_{1}\pm1|\), and \(|\ell_{i}|=|k_{i}|\).
Thus, \(|\ell+v|_{1}<|k+v|_{1}\), and they are clearly neighbors, so since \(q\) is volcanic, \(q(k+v)\leq q(\ell+v)=q(k+e_{1}+v)\). By the local monotonicity of \(\mathcal{S}\), this implies that \(\mathcal{S}q(k)\leq \mathcal{S}q(k+e_{1})=\mathcal{S}q(\ell)\), as desired.
Case 2. \(\ell_1 = 0\). In this case, the analysis is more delicate. Using the symmetry of \(q\), without loss of generality, we may write \(\ell= (0, \ldots, 0, \ell_{m+1}, \ldots, \ell_d)\), where \(m\geq 1\) denotes the number of zero coordinates of \(\ell\).
Since \(q\) is volcanic and \(k\) and \(\ell\) are neighbours with \(|k|_{1}> |\ell|_{1}\), \(q(k)\leq q(\ell)\). To prove the desired claim, we compute \[\begin{align} &\mathcal{S}q(\ell) - \mathcal{S}q(k)\\ &=q(\ell)-q(k)+{1\over2d}\sum_{i=1}^{m}[A(q(\ell\pm e_{i}))-A(q(\ell))]-{1\over2d}\sum_{i=1}^{m}[A(q(k\pm e_{i}))-A(q(k))]\\ &\quad +{1\over2d}\sum_{i=m+1}^{d}[A(q(\ell\pm e_{i}))-A(q(\ell))]-[A(q(k\pm e_{i}))-A(q(k))] \end{align}\]
We will analyze each of the above sums separately. By symmetry, we have that for all \(1\leq i\leq m\), \(q(\ell\pm e_{i}) = q(\ell+e_{1})=q(k)\), so \[\label{monotonezeropiecea} R_1 := {1\over2d}\sum_{i=1}^{m}[A(q(\ell\pm e_{i}))-A(q(\ell))] = {2m \over 2d} [A(q(k)) - A(q(\ell))].\tag{20}\]
For the next term, we note that for \(1< i\leq m\), \(|k\pm e_{i}|_{1}>|k|_{1}\) and \(|k+e_{1}|_{1}>|k|_{1}\). Since \(q\) is volcanic and \(A'\geq 0\), we have \(A(q(k+v))-A(q(k))\leq 0\) for all \(v\sim 0\) with \(v\neq -e_{1}\). This implies \[\begin{align} R_2 :=-{1\over2d}\sum_{i=1}^{m}[A(q(k\pm e_{i}))-A(q(k))]&\geq -\frac{1}{2d}[A(q(k-e_{1})-A(q(k))]\\ &=\frac{1}{2d}[A(q(k))-A(q(\ell))]. \end{align}\]
For the last term, we observe that for \(m+1\leq i\leq d\), \(|k\pm e_{i}|_{1}>|\ell\pm e_{i}|_{1}\), and thus by the same argument as in the last step, \(A(q(\ell\pm e_{i})) - A(q(k\pm e_{i})) \ge 0.\) This implies \[\begin{align} \label{monotonezeropiecec} R_3 &:={1\over2d}\sum_{i=m+1}^{d}[A(q(\ell\pm e_{i}))-A(q(\ell))]-[A(q(k\pm e_{i}))-A(q(k))]\notag\\ &\geq {1\over2d}\sum_{i=m+1}^{d}[A(q(k))-A(q(\ell))]={2d - 2m \over 2d} [A(q(k))-A(q(\ell))] \end{align}\tag{21}\] Adding up the three prior inequalities, we get the bound \[\begin{align} \mathcal{S}q(\ell)-\mathcal{S}q(k) &= q(\ell)-q(k) + R_{1}+R_{2}+R_{3} \\&\ge q(\ell)-q(k) + {2d+1 \over 2d} [A(q(k))-A(q(\ell))]. \end{align}\] Recall that \(q(k) \le q(\ell)\), and since \(0\leq A'(\cdot) \le 2/3\), we have \[0\leq A(q(\ell)) - A(q(k)) \le \frac{2}{3} (q(\ell) - q(k)).\] Therefore, since \(d>1\), we conclude \[\begin{align} \mathcal{S}q(\ell) - \mathcal{S}q(k) &\ge q(\ell)- q(k) - {(2d + 1) \over 3d}[q(\ell)-q(k)] \\ &\ge [q(\ell)- q(k)]\left[1 - {2d+1 \over 3d}\right] \\&\ge 0, \end{align}\] and this completes the proof. ◻
Corollary 10. If \(A(u) = u^{m+1}\) with \(m \ge 1\), then the scheme (14 ) is volcano-preserving on \(\mathcal{B}^{+}_{\frac{1}{3}}(\mathbb{Z}^{d})\).
Proof. By Lemma 9, we smply need to check that \(0 \le A'(\cdot) \le 2/3\) on the interval \([0,1/3]\).
Since \(A'(u) = (m+1)u^m\), if \(u \le 1/3\), then \(A'(u)\) decreasing in \(m\) for \(m \ge 1\), because \[\begin{align} {\partial A'(u) \over \partial m}=(1 + (m+1) \ln u) u^m\le (1 + 2\ln u) u^m\le 0. \end{align}\] Therefore \((m+1)u^m \le (1+1)u^1 \le 2/3\). So \(A'(u) \le 2/3\) as long as \(u \in [0, 1/3]\) and the result follows.0◻
\[\bar{u}(x,t):=t^{-d\beta}(C-\gamma|x|^{2}t^{-2\beta})_{+}^{\frac{1}{m}},\] where \(\beta=\frac{1}{dm+2}\) and \(\gamma=\frac{m\beta}{2(m+1)}\), and \(C\) is chosen so that \(\int \bar{u}(x,t)\, dx=1\) for all \(t\).
This is the unique distributional solution (see Section 6.2) to \[\label{e46pmdelta} \begin{cases} u_{t}-\frac{1}{2d}\Delta(u^{m+1})=0&\text{in \mathbb{R}^{d}\times (0, \infty)},\\ u(x,0)=\delta(x)&\text{in \mathbb{R}^{d}}, \end{cases}\tag{22}\] where \(\delta\) here is the Dirac delta. A reference for the construction of the Barenblatt solution is given in [6].
We notice that the parameter \(C\) is used to tune the mass of the solution. Moreover, we also note that for any \(t_{0}\geq 0\), \(\bar{u}(\cdot,\cdot+t_{0})\) solves the PME with initial condition \(\bar{u}(\cdot, t_{0})\). This implies that we can think of the Barenblatt solutions as a 2-parameter family of solutions to the PME.
Instead of parametrizing by the mass and a time-shift, we now write this family in terms of different parametrizations which are better suited for our analysis. Let \(R, \Gamma\) be positive real parameters. We now define \[\label{hformula0}\bar{u}^{(R,\Gamma)}(x, t) := {R^d \Gamma \over r(t)^d} \left(1 - \left({|x| \over r(t)}\right)^2\right)^{1/m}_+,~ r(t) := R \left(1 + {t \over {T_0}}\right)^\beta,~ {T_0}:= {2d\gamma R^2 \over \Gamma^m},\tag{23}\] where we recall \(\beta=\frac{1}{dm+2}\) and \(\gamma=\frac{m\beta}{2(m+1)}\).
It is clear that the function \(\bar{u}^{(R,\Gamma)}(\cdot, t)\) is positive in the open ball \(|x| < r(t)\), and 0 outside it. As such, we call \(B_{r(t)}\) the positive region, and its complement the zero region. The parameters have clear meanings: \(R = r(0)\) is the radius of the positive region at time zero, and \(\Gamma = \bar{u}^{(R,\Gamma)}(0, 0)\) is the largest possible value of \(\bar{u}\) (for all \(x, t\)).
Lemma 11. For each \(R, \Gamma>0\) the Barenblatt solution \(\bar{u}=\bar{u}^{(R,\Gamma)}\) satisfies the following properties:
(i) For \(m>0\), fixed \(x\), \(t\mapsto \bar{u}(x,t)\) is unimodal (i.e. \(\max_{t} \bar{u}(x,t)\) is unique).
(ii) For \(m\geq 1\), for any \(i\in [d]\), \({\partial^4 \over \partial x_i^4} \bar{u}(x,t)\geq 0\) for all \(|x|<r(t)\).
Proof of Lemma 11. To prove the unimodality claim, we recall that for fixed \(x\), \(\bar{u}(x,\cdot)\) could be initially 0, and once there exists \(T\) such that \(|x|<r(T)\), then \(\bar{u}(x,t)\) is strictly positive for all times \(t\geq T\) (so the time derivative must be positive at time \(T\)). We now compute \(\tfrac{\partial\overline{u}}{\partial t}(x,t)\) assuming that \(|x|\leq r(t)\) (since this is where the maximum of \(t\mapsto u(x,t)\) will occur). We introduce the shorthand \(\vartheta := \tfrac{|x|}{r(t)}\) and proceed by logarithmic differentiation. Since \[\log \bar{u}= \log(R^d \Gamma) - d \log r(t) + {1 \over m} \log(1 - \vartheta^2),\] using the fact that \(\tfrac{\partial \vartheta}{\partial t} = -\tfrac{|x|r'(t)}{r(t)^2} = -\tfrac{\vartheta r'(t)}{r(t)}=- \tfrac{\vartheta\beta}{(t + {T_0})}\), and \(md\beta+2\beta=1\), we obtain \[\begin{align} {1 \over \bar{u}} {\partial \bar{u} \over \partial t} &= {-d \beta \over t+T_0} - {1 \over m(1-\vartheta^2)} {\partial\vartheta^2 \over \partial t} \notag \\&={1 \over m(t+T_0)} \left(-md\beta + 2\beta {\vartheta^2 \over 1 - \vartheta^2}\right) \notag \\ &={1 \over m(t+T_0)} \left({1-md\beta \over 1 - \vartheta^2} - 1\right)\notag\\ &={1 \over m(t+T_0)} \left({2\beta \over 1 - \vartheta^2} - 1\right). \label{first46time46derivative} \end{align}\tag{24}\] We conclude that \(\tfrac{\partial\overline{u}}{\partial t}\) has the same sign as \(2\beta(1 - \vartheta^2)^{-1} - 1\), and this is decreasing in time for a fixed \(x\), because \(\vartheta = |x|/r(t)\) is decreasing in time (and less than 1). Therefore, for fixed \(x\), the time derivative of \(\bar{u}(x,t)\) is initially positive and then becomes negative for higher values of \(t\). This implies that \(\bar{u}(x,t)\) is unimodal in \(t\) for a fixed \(x\).
For the second claim, fix \(i\in [d]\), and we begin by rewriting \[{\partial^4 \over \partial x_i^4} \bar{u}^{m+1} = \left({R^d \Gamma \over r(t)^d}\right)^{m+1} {\partial^4 \over \partial x_i^4} \left(s-\left({x_i \over r(t)}\right)^2\right)^{(m+1)/m}_+,\] where \(s := 1 - (\sum_{j \ne i} x_j^2) / r(t)^2\) does not depend on the \(i\)-th coordinate, and thus \(s - x_i^2 / r(t)^2 = 1 - |x|^2/r(t)^2\) is greater than zero by the assumption that \(|x| < r(t)\).
For \(y\in \mathbb{R}\), we make the change of variables \(x_i = s^{1/2} r(t) y\). Then \[{\partial^4 \over \partial x_i^4} \bar{u}^{m+1} = C(R, \Gamma, t, x_1, \ldots, x_{i-1}, x_{i+1}, \ldots, x_d) {d^4 \over dy^4} (1-y^2)^{(m+1)/m}\] where \(C({\cdots})\) is a positive constant that depends on everything except \(x_i\). In other words, the sign of \(\partial_i^4 \bar{u}^{m+1}\) will be the same as the sign of \((d/dy)^4 (1-y^2)^{(m+1)/m}\). We also notice that \(s > x_i^2/r(t)^2\), so \(|y| < 1\).
We now calculate1 the fourth derivative of \((1-y^2)^{(m+1)/m}\), given by \[{d^4 \over dy^4} (1-y^2)^{(m+1)/m} = {4(1+m) (1-y^2)^{1/m-3} \over m^4} (3m^2+(6m^2-12m)y^2+(4-m^2)y^4).\] Let \(\psi(y) := 3m^2 + (6m^2-12m)y^{2} + (4-m^2) y^4\) be the factor on the right. Then since \(m\geq 1\), it follows that \(\psi(y)\geq 0\) for all \(|y|\leq 1\).
The other factors are positive, so \((d/dy)^4 (1-y^2)^{(m+1)/m}\) is nonnegative, and \[{\partial^4 \over \partial x_i^4} \bar{u}^{m+1} = C {d^4 \over d^4y} (1-y^2)^{(m+1)/m} \ge 0.\] This inequality proves the claim about the fourth derivative. ◻
The main goal of this section is to prove the following result. Recall that \(\beta=\tfrac{1}{dm+2}\).
Theorem 12. Let \(\tilde{p}=(\tilde{p}(\cdot, n))_{n\geq n_{0}}\) be a solution of 14 on \([n_{0}, \infty)\) with initial condition \(\tilde{p}_{n_{0}}\). Assume that \(\tilde{p}(\cdot, n)\in \mathcal{B}^{+}_{\frac{1}{3}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\) and \(\tilde{p}(\cdot, n)\) is volcanic for every \(n\geq n_{0}\). If there are positive constants \(C\) and \(N\) so that for all \(n \ge N\), \[\tilde{p}(k, n) \ge Cn^{-d\beta}\quad\text{for all |k| \le Cn^\beta},\] Then there is a constant \(C'=C'(C, d,m, |\tilde{p}_{n_{0}}|_{1},N)>0\) such that for all \(n\geq N\), \[\sup_{k\in\mathbb{Z}^d} \tilde{p}(k,n)\le C'n^{-d\beta}.\]
Theorem 12 will be used to prove Theorem 2(i). The key to establishing Theorem 12 is to interpret solutions of 14 as a type of lazy random walk. This interpretation will allows us to control the values of \(\tilde{p}\) with an associated optimization problem (see Lemma 14 for a precise statement.)
We begin by introducing the framework of lazy random walks. Let \(n_0\in \mathbb{N}_{0}\). Fix functions \(r: \mathbb{Z}^d \times \mathbb{\{}n_0, n_0+1,\ldots \} \to [0, 1]\) and a probability mass function \(h: \mathbb{Z}^d \to [0,1]\). We now define the \(r\)-lazy random walk \((Z_n)_{n\geq n_{0}}\) on \(\mathbb{Z}^d\), started from an initial distribution \(h\), as follows.
The starting location is a random point \(Z_{n_0}\) in \(\mathbb{Z}^d\) such that \({\mathbf{P}}\left\{Z_{n_0}= k\right\} = h(k)\) (we write this as \(Z_{n_{0}}\sim h\)). We define the random walk recursively. At every time step, we choose a neighbour of \(Z_n\) uniformly at random, and call it \(Y_n\). Then \[Z_{n+1} = \begin{cases}Y_n&\text{with probability }r(Z_n,n)\\Z_n&\text{ otherwise}.\end{cases}\] We highlight that the jump probability of the lazy random walk depends on both its location and the time the random walker steps.
Writing \[{\mathbf{P}}\left\{Z_{n+1} = k\right\} = \sum_{\ell\in \mathbb{Z}^d} {\mathbf{P}}\left\{Z_n = \ell\right\} {\mathbf{P}}\left\{Z_{n+1} = k \mid Z_n = \ell\right\}\, ,\] by the definition of \(Z_{n+1}\), we see that \[{\mathbf{P}}\left\{Z_{n+1} = k \mid Z_n = \ell\right\}=\begin{cases} 1 - r(k, n)&\text{if \ell= k,}\\ \frac{1}{2d}r(\ell, n)&\text{if \ell\sim k,}\\ 0&\text{otherwise.} \end{cases}\] Letting \(f(k, n):= {\mathbf{P}}\left\{Z_n = k\right\}\), we obtain \[\begin{align} \notag\label{lin}f(k, n+1) &= (1 - r(k, n))f(k, n) + \frac{1}{2d}\sum_{\ell\sim k} r(\ell, n) f(\ell, n) \\&= f(k,n) + {1 \over 2d} \sum_{\ell\sim k} \left[r(\ell,n) f(\ell,n) - r(k,n) f(k,n)\right]. \end{align}\tag{25}\] This recurrence has a unique solution for a given initial condition \(f(k, n_0) = h(k)\). Here, we see that functions \(r(k,n)\), corresponding to the jump probabilities, act effectively as diffusivity parameters in this model.
Thus, we see that a \(\mathop{\mathrm{CM}}(m,d)\)-cooperative motion \(X=(X_n)_{n\geq 0}\) is a lazy random walk started from \(\boldsymbol{1}_{0}\), with \(r(k, n) = p(k, n)^{m}\). Moreover, if we have any solution \(\tilde{p}\) of the scheme 14 on any domain, and we set \(r(k, n) = \tilde{p}(k, n)^m\), then \(f(k, n) = \tilde{p}(k, n)\) solves the above recurrence (25 ).
Let \(Z=(Z_n)_{n\geq n_{0}}\) be a lazy random walk as described above, with jump probability \(r(k, n)\) that varies with space and time. We will introduce an optimization problem over these walks and use it to get a bound on solutions of 14 .
We fix starting and ending times \(n_0 < n_1\) and a fixed volcanic initial distribution \(h(k)\) with \(Z_{n_0} \sim h\). Loosely speaking, our goal is to choose a jump probability function \(r(k, n)\) that maximizes the probability \({\mathbf{P}}\left\{Z_{n_1} = 0\right\}\) of being at the origin at time \(n_1\).
However, for the problem to be useful in our setting, we add some more conditions as follows. We are given two more parameters: a radius \(\rho > 0\) and a jump probability \(b\in [0, 2/3]\). We will only allow jump probability functions \(r=(r(k, n))_{n}\) that satisfy the following three conditions for every time step \(n \in \{n_0, \ldots, n_1 - 1\}\). \[\label{e46rconds} \begin{align} &\text{(i) r(\cdot, n) is volcanic; } \\&\text{(ii) {\mathbf{P}}\left\{Z_n = \cdot\right\} is volcanic for volcanic initial data; } \\&\text{(iii) r(k, n) \ge b for any point k\in \mathbb{Z}^d with |k| \le \rho.} \end{align}\tag{26}\] The second condition is a restriction on \(r(k, n)\) because as can be seen by the recursion, \({\mathbf{P}}\left\{Z_n = k\right\}\) depends continuously on the initial distribution and the jump probabilities.
We first show that it is possible to satisfy all these conditions by taking \(r \equiv b\).
Lemma 13. The constant jump probability \(r \equiv b\) satisfies all three conditions (26 ).
Proof. The first and third conditions are obviously satisfied. For the second condition, we must check that the probabilities \({\mathbf{P}}\left\{Z_n = k\right\}\) are volcanic when \(r \equiv b\).
By assumption, the initial condition \(h\) is volcanic. We observe that the sequence of functions \(q=(q_n(\cdot))_{n_{0}\leq n\leq n_{1}}\) given by \(q_{n}(k) := {\mathbf{P}}\left\{Z_n = k\right\}\) is a solution of 13 on \([n_{0}, n_{1}]\), with \(A(u) = bu\) and initial condition \(h\). Then since \(A'(\cdot) = b \in [0, 2/3]\), Lemma 9 tells us that volcanicity is preserved. Hence, \(q_n(k) = {\mathbf{P}}\left\{Z_n = k\right\}\) is volcanic for \(n_0 \le n < n_1\), and the second condition is also satisfied. ◻
We now try to solve the following optimization problem:
Let \(V^{(\rho, b)}_{n_0 \to n_1}(h)\) be the optimal value in this problem: \[V^{(\rho, b)}_{n_0 \to n_1}(h) := \sup\left\{\vphantom{}{\mathbf{P}}\left\{Z_{n_1} = 0 \mid Z_{n_0} \sim h\right\}\;\middle\vert\;r\text{ satisfies \eqref{e46rconds}}\right\}.\] This value depends on all the parameters \(\rho, b, n_0, n_1, h\), but to keep the notation from becoming cluttered, we will drop the superscript \((\rho, b)\) and simply write \(V_{n_0 \to n_1}(h)\).
We begin with a lemma that connects this optimal value to our main goal of the section, the proof of Theorem 12. It gives us an upper bound on \(\tilde{p}\) in terms of \(V_{n_0 \to n_1}\).
Lemma 14. Let \(n_0 \le n_1\) be nonnegative integers. Let \(\tilde{p}: \mathbb{Z}^d \times \{n_0, \ldots, n_1\} \to [0, 1]\) be a function such that \(\tilde{p}=(\tilde{p}(\cdot,n))_{n_{0}\leq n\leq n_{1}}\) is a solution of the scheme (14 ) on \([n_{0}, n_{1}]\) with initial condition \(\tilde{p}(\cdot, n_{0})\), and for all time steps \(n \in \{n_0, \ldots, n_1\}\),
\(\tilde{p}(\cdot, n)\) is volcanic and
\(\tilde{p}(k, n) \ge b^{1/m}\) whenever \(|k| \le \rho\).
Assume the \(\sigma := \sum_k \tilde{p}(k, n_0)<\infty\). Let \(h(k) := \tilde{p}(k, n_0) / \sigma\). Then for all \(k\in \mathbb{Z}^{d}\), \[\tilde{p}(k,n_{1})\leq \sigma V^{(\rho,b)}_{n_0 \to n_1}(h).\]
Proof. Let \((Z_n)_{n_{0}\leq n\leq n_{1}}\) be a lazy random walk with jump probability \(r(k, n) = \tilde{p}(k, n)^m\) and initial distribution \(h\), as defined above. We first observe that \(\tilde{p}(k,n) = \sigma {\mathbf{P}}\left\{Z_n = k\right\}\), because the function \(f(k, n) := \sigma {\mathbf{P}}\left\{Z_n = k\right\}\) satisfies the relation (25 ) with initial condition \(f(k, n_{0}) = \sigma h(k) = \tilde{p}(k, n_{0})\). Since \(\tilde{p}\) also satisfies 25 with the same initial condition, we conclude that the two functions are equal: \(\sigma {\mathbf{P}}\left\{Z_n = k\right\} = \tilde{p}(k, n)\) for \(k\in \mathbb{Z}^d\) and \(n \in \{n_0, \ldots, n_1\}\).
We now argue that \(r(k, n) = \tilde{p}(k, n)^m\) satisfies 26 . Since \(\tilde{p}\) is volcanic for each \(n\in [n_{0}, n_{1}]\), the jump probability \(r(k, n) = \tilde{p}(k, n)^m\) and the distributions \({\mathbf{P}}\left\{Z_n = k\right\}\) are also volcanic for each \(n\in [n_{0}, n_{1}]\), so the first two conditions hold. We have assumed that \(\tilde{p}(k, n) \ge b^{1/m}\) when \(|k| \le \rho\), which implies that \(r(k, n) = \tilde{p}(k, n)^m \ge b\), so the third condition holds and \(r\) satisfies the three conditions 26 .
This tells us that \({\mathbf{P}}\left\{Z_{n_1} = 0\right\}\) is bounded above by \(V_{n_0 \to n_1}(h)\) by definition. Therefore \[\widetilde{p}(0, n_1) = \sigma {\mathbf{P}}\left\{Z_{n_1} = 0\right\} \le \sigma V_{n_0 \to n_1}(h).\] Our assumption that \(\tilde{p}(\cdot, n_{1})\) is volcanic implies in particular that \(\sup_k\tilde{p}(k, n_1) = \tilde{p}(0, n_1)\), so \(\tilde{p}(k,n_1) \le \tilde{p}(0,n_1) \le \sigma V_{n_0 \to n_1}(h)\) for all points \(k\in \mathbb{Z}^d\). ◻
By Lemma 14, it is now clear that if we can obtain an upper bound on \(V^{(\rho,b)}_{n_0 \to n_1}\), then this paves a path to prove Theorem 12. This also allows us to give some intuition as to why Theorem 12 should hold. The hypothesis of the theorem states that on a ball centered at the origin, the jump probabilities \(\tilde{p}(k,n)^{m}\) are sufficiently large. Heuristically, this suggests that the probability of being at the origin cannot be too large. We make these heuristics precise in the rest of this section, and this will give us an upper bound on precisely the quantity \(V^{(\rho,b)}_{n_0 \to n_1}\). This is how we will establish Theorem 12.
In order to make use of Lemma 14, we establish a formula for \(V_{n_0 \to n_1}(h)\) which will hold as long as \(n_{1}-n_{0}\) is less than a quantity \(T(\rho, b)\) called the breakdown time. We then show that the supremum in \(V_{n_0 \to n_1}(h)\) is in fact attained by a lazy random walk with constant jump probability \(b\).
For \(f: \mathbb{Z}^d \to \mathbb{R}\), recall that the discrete Laplacian \(\Delta f: \mathbb{Z}^d \to \mathbb{R}\) is defined by \[(\Delta f)(k) = \sum_{\ell\sim k} (f(\ell) - f(k)).\]
We first collect some identities for the discrete Laplacian, which we will use throughout this section. We think of the lattice \(\mathbb{Z}^d\) as the vertex set of a directed graph with nearest-neighbour edges \((k, k\pm e_i)\) for \(k\in \mathbb{Z}^d\) and \(i\in [d]\). Each vertex has \(2d\) edges out and \(2d\) edges in. Let \(\sum_{e = (k, \ell)}\) denote the sum over all directed edges.
The discrete gradient is the function \(\nabla f(e) = f(\ell) - f(k)\) on directed edges \(e = (k, \ell)\).
Lemma 15. Let \(f,g:\mathbb{Z}^{d}\to\mathbb{R}\), and suppose at least one of \(f\) and \(g\) has bounded support. Then we have
(i) Green’s identity: \[\sum_{k\in \mathbb{Z}^{d}} \Delta f(k) g(k) = \sum_{k\in \mathbb{Z}^{d}} f(k) \Delta g(k).\]
(ii) Discrete integration by parts: \[\sum_{e~\text{an edge of}~\mathbb{Z}^d} \nabla f(e) \nabla g(e) = -2\sum_{k\in\mathbb{Z}^{d}} f(k) \Delta g(k).\]
(iii) Product rule: for \(e=(k,\ell)\), \[\nabla(fg)(e) = f(\ell) \nabla g(e) + g(k) \nabla f(e)\]
Proof of (i). By symmetry and the definition of the discrete Laplacian, \[\begin{align} \sum_{k\in \mathbb{Z}^{d}} \Delta f(k) g(k) &= \sum_{k\in \mathbb{Z}^{d}} \sum_{\ell\sim k} f(\ell) g(k) - 2d\sum_{k\in \mathbb{Z}^{d}}f(k) g(k) \\&= \sum_{k\in \mathbb{Z}^{d}} \sum_{\ell\sim k} f(k) g(\ell) - 2d\sum_{k\in \mathbb{Z}^{d}} f(k) g(k) \\&=\sum_{k\in \mathbb{Z}^{d}} f(k) \Delta g(k) \end{align}\] The infinite sums are all well-defined by the assumption of bounded support. ◻
Proof of (ii). We check:\[\begin{align} \sum_e \nabla f(e) \nabla g(e) &=\sum_{k\in \mathbb{Z}^{d}} \sum_{\ell\sim k} (f(\ell) - f(k)) (g(\ell) - g(k)) \\&= 4d \sum_{k\in \mathbb{Z}^{d}} f(k) g(k) - 2\sum_{k\in \mathbb{Z}^{d}} \sum_{\ell\sim k} f(k) g(\ell) \\&= - 2\sum_{k\in \mathbb{Z}^{d}} f(k) \Delta g(k), \end{align}\] where in the second line we switch \(\ell\) and \(k\) in two of the sums. ◻
Proof of (iii). We expand both sides: \[\begin{align} \nabla(fg)(e) &= f(\ell)g(\ell) - f(k) g(k)\\ f(\ell) \nabla g(e) + g(k) \nabla f(e) &= f(\ell) g(\ell) - f(\ell) g(k) + g(k) f(\ell) - g(k) f(k) \end{align}\] and \(-f(\ell) g(k) + g(k) f(\ell) = 0\), so the two lines are the same. ◻
With the discrete Laplacian notation, the recurrence (25 ) can be rewritten as \[f_{n+1} = f_n + \frac{1}{2d}\Delta(r_n f_n),\] where \(f_n(k)=f(k,n)\) and \(r_n(k)=r(k,n)\).
Let \((Y_{n})_{n\geq 0}\) be a lazy random walk with constant jump probability \(b\) and initial distribution \(\boldsymbol{1}_{0}\). We call this a \(b\)-lazy random walk. Let \(q^{(b)}_n(k) := \mathbb{P}[Y_n = k]\). Then \(q_n^{(b)}\) satisfies the recurrence \(q_{n+1}^{(b)} = q_n^{(b)} + \tfrac{b}{2d}\Delta q_n^{(b)}\), and for each \(n\), \(q_{n}^{(b)}\) has bounded support. We will see later that the discrete Laplacian \(q_n^{(b)}(k)\) is nonnegative in a certain region of space/time. In order to express this region precisely, let the breakdown time \(T(\rho, b)\) be given by \[\label{defoftrb} T(\rho, b) := \min\left\{n \ge 0: \text{there exists } k \in \mathbb{Z}^d \text{ with }|k| > \rho \text{ and }\Delta q^{(b)}_n(k) < 0\right\}.\tag{27}\]
We now calculate the exact value of \(V_{n_0 \to n_1}\) when \(n_1 - n_0 \le T(\rho, b)\). Our argument breaks down when the time gap is larger, hence the name “breakdown time.”
Theorem 16. Let \(\rho \ge 0\) and \(b \in [0, 2/3]\). Let \(q^{(b)}=(q_{n}^{(b)})_{n\geq 0}\) be the distribution of a \(b\)-lazy random walk as above. For all nonnegative integers \(n_0 \le n_1\) with \(n_1 - n_0\leq T(\rho, b)\), for any volcanic probability mass function \(h: \mathbb{Z}^d \rightarrow [0,1]\), \[V_{n_0 \to n_1}(h) = \sum_{k\in \mathbb{Z}^{d}} h(k) q^{(b)}_{n_1 - n_0}(k).\]
Proof of Theorem 16. For ease of notation, we write \(q_{n}(k) = q^{(b)}_n(k)\) and \(r_n(k) = r(k, n)\).
We claim that for all \(n\in \left\{n_{0}, n_{0}+1, \ldots, n_{1}\right\}\), \[\label{optiminduction} V_{n \to n_1}(h) = \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1-n}(k).\tag{28}\] We will prove this by induction downward in \(n\), starting from the base case \(n = n_1\) where \(V_{n_1 \to n_1}(h) = h(0)\) and the statement is obvious.
Suppose \(n\in [n_{0}, n_1)\). We know by the induction assumption that \[V_{(n+1) \to n_1}(h) = \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 - (n+1)}(k).\]
We will regard optimization of the jump probabilities \(r\) as an optimal control problem: instead of choosing \(r\) for all values of \(k\) and \(n\), we will choose \(r(k, n)\) at the current step \(n\) and then we will choose \(r(k, n')\) for \(n < n' \le n_1 - 1\). By the Bellman optimality principle, we can find \(V_{n \to n_1}(h)\) by choosing the jump probability \(r_n\) that gives us the best value at step \(n+1\).
If the lazy random walk \(Z_n\) has \({\mathbf{P}}\left\{Z_n = k\right\} = h(k)\), then the distribution of \(Z_{n+1}\) is \[\begin{align} {\mathbf{P}}\left\{Z_{n+1} = k\right\} = h(k) + {1 \over 2d} \sum_{\ell\sim k} \left[r(\ell, n) h(\ell) - r(k, n) h(k)\right]= h(k) + \frac{1}{2d} \Delta(r_nh)(k). \end{align}\] We can now ask about the value of the optimal control problems at time step \(n + 1\), starting from these new distributions. We consider the set of jump probabilities \(r_n: \mathbb{Z}^d \to [0, 1]\) that satisfy the following three conditions: \[\label{e46rcondstwo} \text{(i) r_n is volcanic; } \quad \text{(ii) h +\tfrac{1}{2d} \Delta(r_n h) is volcanic; } \quad \text{(iii) r_n(k) \ge b for |k| \le \rho}.\tag{29}\] We highlight that 29 is a condition for only \(r_{n}\), whereas 26 is a condition for \(r=(r_{n})_{n_{0}\leq n\leq n_{1}-1}\), as well as on \({\mathbf{P}}\left\{Z_{n}=\cdot\right\}\) for \(n\in \left\{n_{0}, \ldots, n_{1}-1\right\}\).
Let \[v := \sup_{r_n} V_{(n+1) \to n_1}\left(h + {1 \over 2d} \Delta(r_n h)\right) = \sup_{r_n} \sum_{k\in \mathbb{Z}^{d}} \left(h(k) + {1 \over 2d}\Delta(r_n h ) \right) q_{n_1 - (n+1)}(k),\] where we take the supremum over jump probabilities \(r_n\) that satisfy 29 , and the second equality holds by the induction hypothesis.
We claim that \(V_{n \to n_1}(h) = v\). To prove this, we show that \(V_{n \to n_1}(h) \le v\) and that \(v \le V_{n \to n_1}(h)\) separately. First, if \(r\) is a jump probability that satisfies the conditions 26 with initial time \(n\), then \(r\) satisfies 26 with initial time \(n+1\) and starting distribution \(h(k) = {\mathbf{P}}\left\{Z_{n+1} = k\right\} = h + \tfrac{1}{2d} \Delta(r_n h)\). Thus,\[{\mathbf{P}}\left\{Z_{n_1} = 0\right\} \le V_{(n+1) \to n_1}\left(h + {1 \over 2d} \Delta(r_n h)\right) \le v,\]because \(r_n\) satisfies the conditions 29 . Therefore \(V_{n \to n_1}(h) \le v\).
Conversely, if \((r_{n'})_{n+1\leq n'\leq n_{1}}\) satisfies 26 , and \(r_{n}\) satisfies 29 , then we claim that \((r_{n'})_{n\leq n'\leq n_{1}}\) satisfies 26 . Indeed, \({\mathbf{P}}\left\{Z_{n}=\cdot\right\}=h\) is volcanic, and \({\mathbf{P}}\left\{Z_{n+1}=\cdot\right\}=h+\frac{1}{2d}\Delta h\) is volcanic by property (ii) of 29 . Hence, we have that \[V_{(n+1) \to n_1}\left(h + {1 \over 2d} \Delta(r_n h)\right)\leq V_{n \to n_1}\left(h\right),\] and taking a supremum over \(r_{n}\) satisfying 29 , we obtain that \(v\leq V_{n \to n_1}\left(h\right)\).
We next prove that \(v = \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 -n}(k)\), which will give us the conclusion. By Lemma 13, constant jump probability \(r_n \equiv b\) satisfies all three conditions 29 , so \[\begin{align} \notag \sum_{k\in \mathbb{Z}^d} h(k) q_{n_1 - n}(k) &= \sum_{k\in \mathbb{Z}^{d}} h(k) \left( q_{n_1 - (n+1)}(k) + {b \over 2d} \Delta q_{n_1 - (n+1)}(k) \right) \\\label{e46achieved} &= \sum_{k\in \mathbb{Z}^{d}} \left(h(k) + {1 \over 2d} \Delta(bh)\right) q_{n_1 - (n+1)}(k), \end{align}\tag{30}\] where in the first line, we use the recurrence \(q_{n+1} = q_n + (b/2d) \Delta q_n\), and in the second line, we use part (i) of Lemma 15. Therefore, \(\sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 - n}(k) \le v\).
We now prove that \(\sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 - n}(k) \ge v\), which is more difficult and requires the hypothesis that \(n_1 - n_0 \le T(\rho, b)\). We will first show that it is enough to consider functions \(r_n\) with \(r_n \ge b\) pointwise everywhere, and then show that \(r_n \equiv b\) is an optimal choice.
Suppose \(r_{n}:\mathbb{Z}^d \to [0, 1]\) is a jump probability that satisfies conditions 29 (i) and 29 (iii). Our inductive hypothesis tells us that \[\label{e46valueinductivehypothesis}V_{(n+1) \to n_1}\left(h + {1 \over 2d}\Delta(r_nh)\right) = \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 - (n +1)}(k) + {1 \over 2d} \sum_{k\in \mathbb{Z}^{d}} \Delta(r_nh)(k) q_{n_1 - (n + 1)}(k).\tag{31}\] We will focus on analyzing the second term in the sum. We use the first part of Lemma 15(i) to move the discrete Laplacian to the other factor: \[\label{value46one}\frac{1}{2d}\sum_{k\in \mathbb{Z}^{d}} \Delta(r_nh)(k) q_{n_1 - (n + 1)}(k) = \frac{1}{2d}\sum_{k\in \mathbb{Z}^{d}} r_n(k) h(k) \Delta q_{n_1 - (n + 1)}(k).\tag{32}\]
Consider the modified jump probability \(r'(k) := r_n(k) \vee b\). Then we claim that for any \(k\in \mathbb{Z}^d\), \[r_n(k) h(k) \Delta q_{n_1 - (n + 1)}(k) \le r'(k) h(k) \Delta q_{n_1 - (n + 1)}(k).\] To see this, note that the two sides are equal for \(|k| \le \rho\), because \(r_n\) satisfies the third condition of 29 . On the other hand, if \(|k| > \rho\), then the discrete Laplacian \(\Delta q_{n_1 - n - 1}(k)\) is nonnegative by definition of \(T(\rho, b)\), and \(h \ge 0\) and \(r' \ge r_{n}\), so the relation also holds. Summing this up over all \(k\), we have \[\sum_{k\in \mathbb{Z}^{d}} r_n(k) h(k) \Delta q_{n_1 - (n + 1)}(k)\le \sum_{k\in \mathbb{Z}^{d}} r'(k) h(k) \Delta q_{n_1 - (n + 1)}(k).\] We now perform integration by parts on the term on the right, using Lemma 15(ii) and (iii), \[\begin{align} &\sum_{k\in \mathbb{Z}^{d}} r'(k) h(k) \Delta q_{n_1-(n+1)}(k) \\&\qquad\qquad = - \frac{1}{2}\sum_{e=(k,\ell)} \nabla(r'h)(e) \nabla q_{n_1-(n+1)}(e) \\&\qquad\qquad = - \frac{1}{2}\left(\sum_{e=(k,\ell)} r'(\ell) \nabla h(e) \nabla q_{n_1-(n+1)}(e) + \sum_{e=(k,\ell)} h(k) \nabla r'(e) \nabla q_{n_1-(n+1)}(e)\right), \end{align}\]
The functions \(r', h, q_{n_1-(n+1)}\) are volcanic, the first two by assumption and the last one by Lemma 13. This determines the sign of the discrete gradient across any edge. For example, \(r'(\ell) - r'(k)\) has the same sign as \(h(\ell) - h(k)\). Therefore, the products of two discrete gradients in the above sums are nonnegative. This means that the second sum is nonnegative, and \(r' \ge b\), so the whole expression in brackets is at least \(\sum_e b \nabla h(e) \nabla q_{n_1 - (n+1)}(e)\). Because there is a minus sign in front, we obtain the upper bound, \[\begin{align} \sum_{k\in \mathbb{Z}^d} r'(k) h(k) \Delta q_{n_1-(n+1)}(k) &\le -\frac{1}{2} \sum_{e=(k,\ell)} b \nabla h(e) \nabla q_{n_1-(n+1)}(e) \\&= b \sum_{k\in \mathbb{Z}^d} h(k) \Delta q_{n_1-(n+1)}(k), \end{align}\] where in the last step, we performed another integration by parts using Lemma 15(ii). We now put all this together. By 31 and the inequality we have just proved, \[\begin{align} V_{(n+1) \to n_1}\left(h + {1 \over 2d} \Delta(r_n h)\right) &\le \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1-(n+1)}(k) + \frac{1}{2d}\sum_{k\in \mathbb{Z}^{d}} r'(k) h(k)\Delta q_{n_1-(n+1)}(k) \\&\le \sum_{k\in \mathbb{Z}^{d}} h(k) q_{{n_1}-(n+1)}(k) + \frac{1}{2d} \sum_{k\in \mathbb{Z}^{d}} b h(k) \Delta q_{{n_1}-(n+1)}(k) \\&=\sum_{k\in \mathbb{Z}^d} h(k) \left(q_{n_1 - (n+1)}(k) + {b \over 2d} \Delta q_{n_1 - (n+1)}(k)\right) \\&=\sum_{k\in\mathbb{Z}^d} h(k) q_{n_1 - n}(k). \end{align}\] We have proven the above bound for any jump probability \(r_n\) which satisfies 29 (i) and 29 (iii), so it certainly also holds for jump probabilities \(r_n\) which satisfy all three conditions of 29 . Taking the supremum over all such \(r_n\), we get \(v \le \sum_{k\in \mathbb{Z}^d} h(k) q_{n_1 - n}(k)\).
Finally, we conclude that \[V_{n \to n_1}(h) = v = \sum_kh(k) q_{n_1 - n}(k).\] This verifies the induction step, so the formula is true for all \(n \in \{n_0, \ldots, n_1\}\), and in particular it is true for \(n_0\), which gives us the result \(V_{n_0 \to n_1}(h) = \sum_{k\in \mathbb{Z}^{d}} h(k) q_{n_1 - n_0}(k)\). ◻
In order to prove Theorem 12, we will require an auxiliary result which gives us a bound on the breakdown time \(T(\rho, b)\), as defined in 27 .
Theorem 17. There are positive constants \(\Lambda=\Lambda(d)\) and \(k_2=k_{2}(d,m)\) such that, if \(b\leq \tfrac{1}{8}\), and \(q^{(b)}=(q_{n}^{(b)})_{n\geq 0}\) be a \(b\)-lazy random walk, then for all \(|k| \ge k_2\), and \(n \le \Lambda \tfrac{|k|^2}{6b}\), \[q^{(b)}_n(k) \le q^{(b)}_{n+1}(k).\]
The proof of Theorem 17 can be found in Section 7; it yields the following lower bound on the breakdown time.
Corollary 18. Let \(T(\rho,b)\) be defined as in 27 . There exist positive constants \(c=c(d,m)\) and \(\rho_{0}=\rho_{0}(d,m)\) such that for any \(b\leq \tfrac{1}{8}\) and \(\rho\geq \rho_{0}\), \(T(\rho,b) \ge c\rho^{2}b^{-1}\).
Proof. Let \(q_{n}^{(b)}\) be defined as in the text above 27 . The discrete Laplacian is \[\Delta q_{n-1}^{(b)}(k) = \sum_{\ell\sim k} q_{n-1}^{(b)}(\ell) - q_{n-1}^{(b)}(k) = \frac{2d}{b}\left(q^{(b)}_n(k) - q^{(b)}_{n-1}(k)\right)\] and by Theorem 17, this is nonnegative if \(|k| \ge k_2\) and \(n-1 \le \Lambda |k|^2/6b\). This implies the corollary with \(c = \Lambda/6 = 1/48d^4\) and \(\rho_0 = k_2\). ◻
We may now combine all of the prior results to prove Theorem 12.
Proof of Theorem 12. By the hypotheses, there are positive constants \(C, \beta\) and \(N\) so that for \(n \ge N\), \[\tilde{p}(k, n) \ge Cn^{-d\beta}\quad\text{for all |k| \le Cn^\beta},\] where \(\tilde{p}(\cdot, n)\) is volcanic for each \(n\).
Fix \(n_{1}\geq (2N)\vee (2C^{m})^{\tfrac{1}{dm\beta}}\) and let \(\rho := C(n_{1}/2)^\beta\). By the above, we have \[\tilde{p}(k,j)^m\geq \frac{C^{m}}{n_{1}^{dm\beta}}=:b\quad\text{for |k| \le \rho and n_{1}/2 \le j \le n_{1}}.\] Observe that by the choice of \(n_{1}\), \(b\leq \tfrac{1}{2}\).
Let \(n_0:=\tfrac{n_{1}}{2}\vee (n_{1} - T(\rho,b))\), where \(T(\rho,b)\) is as in (27 ), and let \(\sigma := \sum_{k\in \mathbb{Z}^{d}} \tilde{p}(k, n_0)\). Given that \(\tilde{p}(\cdot,n)\) is volcanic, all hypotheses of Lemma 14 are satisfied. Thus, \[\tilde{p}(k,n_{1})\leq \sigma V^{(\rho, b)}_{n_0 \to n_{1}}(\sigma^{-1}\tilde{p}(\cdot, n_{0})).\] By Theorem 16, this implies that for all \(k\in \mathbb{Z}^{d}\), \[\begin{align} \label{e46pqbd} \tilde{p}(k,n_{1})&\leq \sigma \sum_{k\in \mathbb{Z}^{d}} \sigma^{-1}\tilde{p}(k,n_{0})q^{(b)}_{n_{1} - n_0}(k) \notag \\&\le \sigma \sup_{k\in \mathbb{Z}^{d}} q_{n_{1} - n_0}^{(b)}(k)\notag \\&= \sigma q^{(b)}_{n_{1}-n_0}(0), \end{align}\tag{33}\] where in the last line, we used the fact that by Lemma 9 (with the function \(A(u) = bu\)), \(q_n^{(b)}(k)\) is volcanic, since \(b\leq \tfrac{1}{2}\).
In order to conclude, we simply need to estimate the probability that a \(b\)-lazy random walk \((Y_{n})_{n\geq 0}\) is at \(0\) after some number of steps. We seek an estimate which is uniform in \(b\), and consequently, we will consider the asymptotics of the characteristic function associated to the \(b\)-lazy random walk. After one step, the characteristic function \(\phi\) is given by \[\phi(\vartheta_1, \ldots, \vartheta_d) := {\mathbf{E}}\left[\exp(i Y_1 \cdot \vartheta)\right] = 1 - b + {b \over 2d} \sum_{j=1}^d \cos \vartheta_j.\] Due to the independent increments of the lazy random walk, \(\phi^n\) will be the characteristic function of \(Y_n\), and we can recover the probability that \(Y_n = 0\) by using Fourier series inversion and evaluating at 0, \[q^{(b)}_n(0)={\mathbf{P}}\left\{Y_n = 0\right\} = {1 \over (2\pi)^d} \int_{-\pi}^\pi \cdots \int_{-\pi}^{\pi} \phi^n(\vartheta_1, \ldots, \vartheta_d) \,d\vartheta_1 \cdots d\vartheta_d.\] Now we can use classic asymptotic analysis arguments. Since \(1-x \le e^{-x}\), \[\begin{align} q^{(b)}_n(0) &= {1 \over (2\pi)^d} \int_{-\pi}^\pi\cdots\int_{-\pi}^{\pi} \left(1-b+b\left(\frac{1}{2d}\sum_{i=1}^d \cos \vartheta_i\right)\right)^n \,d\vartheta_1 \cdots \,d\vartheta_d \\&\le {1 \over (2\pi)^d} \int_{[-\pi, \pi]^{d}} \exp\left(-bn\left(1 - \frac{1}{2d}\sum_{i=1}^d \cos \vartheta_i\right)\right) \,d\vartheta. \end{align}\]
Let \(f(\vartheta_1, \ldots, \vartheta_d) := 1 - {1 \over 2d} \sum_{i=1}^d \cos \vartheta_i\). The only minimum of \(f\) in the domain of integration is at \(\vartheta = 0\), where \(f = 0\). By Laplace’s method, we obtain the asymptotic estimate that for \(t\gg 1\), \[H(t) := \int_{[-\pi, \pi]^{d}} \exp(-tf(\vartheta)) \,d\vartheta \sim \frac{K}{t^{d/2}},\] where \(K=K(d)>0\). Since \(H(t)\) is bounded for all \(t\), we conclude that there exists \(K=K(d)\) such that \(H(t) \le K/t^{d/2}\) for all \(t \ge 0\). This constant depends only on \(d\), not on the probability \(b\), and hence \(q^{(b)}_{n}(0)\leq K(bt)^{-\tfrac{d}{2}}\). Continuing from 33 , this implies that \[\tilde{p}(k,n_{1})\leq \frac{K\sigma}{(b(n_{1}-n_{0}))^{d/2}}.\]
Finally, we estimate a lower bound on \(n_{1} - n_0\). By Corollary 18, we have that \(T(\rho, b) \ge c\rho^2/b\), where \(c=c(d,m)\). Therefore, by the choices of \(n_{1}\) and \(n_{0}\), we have \[b(n_{1}-n_0) \ge b\min\{n_{1}/2, T(\rho, b)\}\geq \min\{\tfrac{bn_{1}}{2}, c\rho^2\}=\min\{cn_{1}^{1-dm\beta}, cn_{1}^{2\beta}\}.\] But these are of the same order in \(n\), since \(1 - dm\beta = (dm+2)\beta - dm\beta = 2\beta\). Therefore, for all \(k\in \mathbb{Z}^{d}\), there exists \(C'=C'(C, d,m, \sigma)\) such that \[\tilde{p}(k,n_{1}) \le {K\sigma \over (b(n_{1}-n_0))^{d/2}} \le C'(n_{1}^{-2\beta})^{d/2} = {C' \over n_{1}^{d\beta}}.\] This works for all \(n_{1}\) sufficiently large, depending on \(C, d, m, N\). Finally, by enlarging the constant \(C'=C'(C, d,m, \sigma, N)\), we can obtain the desired estimate for all \(n_{1}\geq N\). ◻
Recall from 4 that \(p(k,n)\) is the probability mass function of \(X^{n}\), where \((X^{n}, n\geq 0)\) is \(\mathop{\mathrm{CM}}(m,d)\)-cooperative motion started from \(0\in \mathbb{Z}^{d}\). As in the prior section, we will frequently write \(p_{n}(k)=p(k,n)\) and consider the sequence of functions \(p=(p_{n})_{n \geq 0}\). The goal in this section is to prove Theorem 2(i), the statement that there exists \(C=C(d,m)>0\) such that \(p(k, n) \le Cn^{-d\beta}\).
While Theorem 12 yields a good approach to proving upper bounds for solutions of 14 which are volcanic in space for each time step (we hereby call such sequences of functions “volcanos”), the sequence \(p=(p_{n})_{n\geq 0}\) is not a volcano. Thus, we begin by first finding a volcano \(\tilde{p}=(\tilde{p}_{n})_{n\geq 0}\) such that \(\tilde{p}_{n}\) lies above \(p_{n}\) for some \(n\) (see Section 4.1.1). In order to verify the hypotheses of Theorem 12 for \(\tilde{p}\), namely a sufficient lower bound in a ball centered at the origin, we compare \(\tilde{p}\) to a discretization of the Barenblatt solution \(\bar{u}=\bar{u}^{(R, \Gamma)}\), for suitably chosen parameters. The discretization of \(\bar{u}\) is not a solution of 14 on \([0, \infty)\), however it turns out that is approximately a solution, in a sense which we make precise below. This leads us to develop a theory of comparison between solutions and approximate solutions, which is how we will establish the desired lower bound on \(\tilde{p}\). By finally applying Theorem 12, we will complete the proof of Theorem 2(i).
Many of the techniques from the prior sections are developed for volcanic functions. The actual probability distribution of cooperative motion at a fixed time is generally not volcanic; for example, \(p_{1}(0) = 0\) and \(p_1(e_1) = (2d)^{-1}\). Instead, we use the following lemma to find a solution \(\tilde{p}=(\tilde{p}_{n})_{n\geq 0}\) of 14 with initial condition \(\tilde{p}_{0}\) such that \(\tilde{p}_{n}\) is volcanic for all \(n\geq 0\) and there exists \(N_{0}\) such that \(\tilde{p}_n(k)\ge{p}_{n+N_{0}}(k)\) for all \(n \ge 0\).
Lemma 19. There exists \(N_{0}=N_{0}(d,m)\in \mathbb{N}\) and a solution \(\tilde{p}_n\) of the scheme (14 ) on \([0, \infty)\) with initial condition \(\tilde{p}_{0}\) such that \(\tilde{p}_{n}\) is volcanic for all \(n\geq 0\), \(|\tilde{p}_0|_1 <\infty\) and \[0 \le p_{n+N_{0}}(k) \le \tilde{p}_n(k) \le \frac{1}{3} \qquad \text{for all }k\in \mathbb{Z}^d, n \ge 0.\]
Proof. Since \(d\geq 2\), \(p_1(k)=(2d)^{-1}\boldsymbol{1}_{\pm e_{i}}(k)\). Set \[\tilde{p}_0(k) = \begin{cases}\frac{1}{2d}&\text{ if k=0, \pm e_{i}}\\0&\text{ otherwise}.\end{cases}\] Then \(\tilde{p}_{0}\) is symmetric and nondecreasing towards the origin. Moreover, \(p_1 \le \tilde{p}_0\le1/3\). Let \(\tilde{p}=(\tilde{p}_{n})_{n\geq 0}\) be a solution of 14 with initial condition \(\tilde{p}_{0}\). Then by Corollary 6, \(p_{n+1} = \mathcal{S}^n p_1 \le \mathcal{S}^n \tilde{p}_0 = \tilde{p}_n\), and by Lemma 9, \(\tilde{p}_n\) is volcanic for every \(n\). This implies the result with \(N_{0} = 1\). Also by Corollary 6, for every \(n\), \[\sum_{k\in \mathbb{Z}^{d}} |\tilde{p}_n(k)| =\sum_{k\in \mathbb{Z}^{d}} |\tilde{p}_0(k)|= (2d)^{-1}(2d+1).\] ◻
We say \(q=(q_{n})_{n\geq 0}\subset \mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\) is a subsolution of 13 on \([n_{0}, \infty)\) with initial condition \(f: \mathbb{Z}^{d}\rightarrow \mathbb{R}\) if \[\begin{cases} q_{n+1} \le \mathcal{S}q_n&\text{for n\geq n_0},\\ q_{n_{0}}=f. \end{cases}\] One can see by induction and Corollary 6 that if \(\tilde{p}=(\tilde{p}_n)_{n\geq 0}\) is a solution of 14 with \(\tilde{p}_{0}\in \mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\), and \(q=(q_n)_{n\geq 0}\) is a subsolution of 14 with initial condition \(q_{0}\), and \(q_{0}\leq \tilde{p}_{0}\), then \(q_{n} \le \tilde{p}_n\) for \(n \ge 0\).
This idea is a little too rigid to be useful for this scheme, so we generalize it and introduce the idea of an approximate subsolution. We begin by defining a distance.
If \(q, r \in \mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\), we define the asymmetric distance \[\mathrm{dist}[q,r] := \sum_{k\in\mathbb{Z}^d}\max\{q(k)-r(k),0\}=\sum_{k\in \mathbb{Z}^{d}} \left(q(k)-r(k)\right)_{+}.\] Intuitively, this measures how much \(q\) sticks up above \(r\). If \(q \le r\) pointwise, then the asymmetric distance is zero.
The asymmetric distance satisfies the triangle inequality, \(\mathrm{dist}[q,r] \le \mathrm{dist}[q,s] + \mathrm{dist}[s,r]\) and \(\mathrm{dist}[q,r] \le |q - r|_1\). As one might expect, it is not symmetric: \(\mathrm{dist}[q,r] - \mathrm{dist}[r,q] = |q|_1 - |r|_1\), which is not in general zero.
We note that the asymmetric distance satisfies basic monotonicity properties on \(\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\). If \(q\leq \tilde{q}\), then for any \(r\), \(\mathrm{dist}[q,r]\leq \mathrm{dist}[q',r]\). Similarly, if \(r\leq r'\), then for any \(q\), \(\mathrm{dist}[q,r']\leq \mathrm{dist}[q,r]\).
For \(q=(q_n)_{n\geq 0}\subset\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\), let \[\mathop{\rm smallest}(q) := \inf_n |q_n|_1.\] This allows us to define an approximate subsolution.
Definition 20. We say sequence \(q=(q_n)_{n\geq 0}\subset\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\) is an approximate subsolution* to 13 on \([0, \infty)\) with initial condition \(q_{0}\) if \[\sum_{n=0}^\infty \mathrm{dist}[q_{n+1},\mathcal{S}q_n] \le \frac{1}{2} \mathop{\rm smallest}(q).\]*
We now show that we can compare approximate subsolutions with solutions, by considering the asymmetric distance (and not total ordering, as in the case of true subsolutions).
Lemma 21. Let \(\tilde{p}=(\tilde{p}_n)_{n\geq 0}\) and \(q=(q_n)_{n\geq 0}\) be sequences in \(\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\), with \(\tilde{p}\) a solution of 14 with initial condition \(\tilde{p}_{0}\) and \(q\) an approximate subsolution of 14 with initial condition \(q_{0}\). Then for any \(n\in {\mathbb{N}_{0}}\), \[\mathrm{dist}[q_n,\tilde{p}_n] \le \mathrm{dist}[q_0,\tilde{p}_0] + \frac{1}{2} \mathop{\rm smallest}(q).\]
Proof. We proceed by induction to show that for any \(n\in {\mathbb{N}_{0}}\), \[\label{eq:errorlemma}\mathrm{dist}[q_n, \tilde{p}_n] \le \mathrm{dist}[q_0, \tilde{p}_0] + \sum_{j=0}^{n-1} \mathrm{dist}[q_{j+1}, \mathcal{S}q_j].\tag{34}\] We consider the base case when \(n = 0\), where the sum is empty and this is the trivial statement that \(\mathrm{dist}[q_0, \tilde{p}_0] \le \mathrm{dist}[q_0, \tilde{p}_0]\).
Suppose (34 ) holds \(n\). Let \(r_n(k) := \min\{\tilde{p}_n(k), q_n(k)\}\). By monotonicity, \(\mathcal{S}r_n \le \mathcal{S}\tilde{p}_n\) and \(\mathcal{S}r_n \le \mathcal{S}q_n\).
Now using the monotonicity property of asymmetric distance, we have \[\mathrm{dist}[q_{n+1},\tilde{p}_{n+1}]=\mathrm{dist}[q_{n+1},\mathcal{S}\tilde{p}_n]\leq \mathrm{dist}[q_{n+1},\mathcal{S}r_n]\leq \mathrm{dist}[q_{n+1},\mathcal{S}q_n] + \mathrm{dist}[\mathcal{S}q_n,\mathcal{S}r_n].\] But \(\mathcal{S}r_n \le \mathcal{S}q_n\), so \(\mathrm{dist}[\mathcal{S}q_n,\mathcal{S}r_n] = |\mathcal{S}q_n - \mathcal{S}r_n |_1\leq |q_n - r_n|_1\) by Corollary 6(iii). Since \(r_n = \min\{\tilde{p}_n, q_n\}\), it follows that \(| q_n - r_n |_1 = \mathrm{dist}[q_n,\tilde{p}_n]\). Therefore, \[\begin{align} \mathrm{dist}[q_{n+1},\tilde{p}_{n+1}] &\le \mathrm{dist}[q_{n+1},\mathcal{S}q_n] + \mathrm{dist}[q_n,\tilde{p}_n] \\[-.9em]&\le \mathrm{dist}[q_{n+1},\mathcal{S}q_n] + \mathrm{dist}[q_0,\tilde{p}_0] + \sum_{j=0}^{n-1} \mathrm{dist}[q_{j+1},\mathcal{S}q_j]\\[-.9em] &=\mathrm{dist}[q_0,\tilde{p}_0]+\sum_{j=0}^{n} \mathrm{dist}[q_{j+1},\mathcal{S}q_j]. \end{align}\] Thus, 34 holds for all \(n\in {\mathbb{N}_{0}}\). Since \(q\) is an approximate subsolution to 14 on \([0, \infty)\) with initial condition \(q_{0}\), we conclude that \[\mathrm{dist}[q_n, \tilde{p}_n] \le \mathrm{dist}[q_0, \tilde{p}_0] + \frac{1}{2}\mathop{\rm smallest}(q). \hfill\qedhere\] ◻
We recall the Barenblatt solution introduced in Section 2.4: \[\label{hformula}\bar{u}^{(R,\Gamma)}(x, t) := {R^d \Gamma \over r(t)^d} \left(1 - \left({|x| \over r(t)}\right)^2\right)^{1/m}_+, \quad r(t) := R \left(1 + {t \over {T_0}}\right)^\beta, \quad {T_0}:= {2d\gamma R^2 \over \Gamma^m},\tag{35}\] where \(\beta=\frac{1}{dm+2}\) and \(\gamma=\frac{m\beta}{2(m+1)}\).
For \(n\in {\mathbb{N}}_{0}\), let \(\bar{u}^{(R,\Gamma)}_n: \mathbb{Z}^d \to \mathbb{R}\) be the function \[\bar{u}^{(R,\Gamma)}_n(k) = \bar{u}^{(R,\Gamma)}(k,n).\] This is the continuous (Barenblatt) solution with discrete integer coordinates plugged in. We will omit the dependence on \(R, \Gamma\) from the notation and simply write \(\bar{u}_n\) and \(\bar{u}(k, n)\). We will always have \(\Gamma<\frac{1}{3}\) and since \(\int \bar{u}(x,t)\, dx<\infty\), \(\bar{u}_n\) belongs to \(\mathcal{B}^{+}_{\frac{1}{2}}(\mathbb{Z}^{d})\cap L^{1}(\mathbb{Z}^{d})\).
The main goal of this subsection is to show that \(\bar{u}=(\bar{u}_{n})_{n\geq 0}\) is in fact an approximate subsolution of 14 with initial condition \(\bar{u}_{0}\), in the sense of Definition 20. Throughout this section, we use the operator \(\mathcal{S}\) given by 12 with \(A(u)=u^{m+1}\). In other words, \[\label{e46bbSdef} \mathcal{S}q(k) := q(k) +\frac{1}{2d}\sum_{\ell\sim k} \left[q(\ell)^{m+1} -q(k)^{m+1}\right].\tag{36}\] We will be interested in estimating \[\label{discretepmeerror} \bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k) = \bar{u}_{n+1}(k) - \bar{u}_{n}(k) - \frac{1}{2d} \sum_{\ell\sim k} \left[ \bar{u}_n(\ell)^{m+1} - \bar{u}_n(k)^{m+1}\right].\tag{37}\]
Proposition 22. For any \(\Gamma\in (0, \frac{1}{3})\), there exists \(R=R(d,m)>0\) such that \(\bar{u}=(\bar{u}_{n})_{n\geq 0}\) as defined in 35 is an approximate subsolution of 14 on \([0, \infty)\) with initial condition \(\bar{u}_{0}\), i.e., for \(\mathcal{S}\) as in 36 , we have \[\sum_{n=0}^\infty \mathrm{dist}[\bar{u}_{n+1},\mathcal{S}\bar{u}_n]=\sum_{n=0}^{\infty} \sum_{k\in \mathbb{Z}^d} (\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_+ \le \frac{1}{2} \mathop{\rm smallest}(\bar{u}).\]
In order to prove Proposition 22, we perform a detailed analysis of the function \(\bar{u}\), and its discretization, in three regions of \(\mathbb{Z}^{d}\times {\mathbb{N}}\). We will consider the core, the gap, and the outer region, respectively defined by \[\label{e46regdefs} \begin{cases} \mathcal{C}:=\left\{(k,n)\in \mathbb{Z}^{d}\times {\mathbb{N}}: |k|<r(n)-\sqrt{d}\right\},\\ \mathcal{G}:=\left\{(k,n) \in \mathbb{Z}^d \times \mathbb{N}: r(n) - \sqrt{d} \le |k| < r(n) + 1\right\},\\ \mathcal{O}:=\left\{(k,n)\in \mathbb{Z}^{d}\times {\mathbb{N}}: |k| \ge r(n) + 1\right\}, \end{cases}\tag{38}\] where we recall that \(|k|\) refers to the Euclidean norm of \(k\in \mathbb{Z}^{d}\). Notice that \(\bar{u}(\cdot, t)\) is supported on \(\overline{B_{r(t)}}\). Outside of the support, \(\bar{u}\) is identically zero, making the discretization \(\bar{u}_{n}\) in the outer region \(\mathcal{O}\) identically zero as well.
In the gap \(\mathcal{G}\), the function \(\bar{u}\) has singular derivatives. The discrete regions we have created give us “some room” which will allow us to control the error in a uniform fashion. For \(|x|<r(t)\), \(\bar{u}\) is smooth, and hence in the core region \(\mathcal{C}\), the analysis of the discretization \(\bar{u}_{n}\) will rely heavily on derivative estimates of \(\bar{u}\), which, to our knowledge, have not previously appeared in the literature.
We estimate the total error in the core, the gap, and the outer region in Proposition 23, Proposition 24 and Proposition 26 respectively. Combining these will straightforwardly yield Proposition 22.
We first start with total error in the outer region \(\mathcal{O}\), which is the most straightforward region to analyze.
Proposition 23. Let \(\Gamma\in (0, \frac{1}{3})\), and any \(R\in [(2d\gamma)^{-1}, \infty)\) where \(\gamma=\gamma(d,m)\) is defined near 35 . For \(\mathcal{O}\) as defined in 38 and \(\mathcal{S}\) as defined in 36 , \[\sum_{(k,n)\in \mathcal{O}} (\bar{u}_{n+1}(k)-\mathcal{S}\bar{u}_{n}(k))_{+}=0.\]
Proof. By definition of \(\bar{u}\), we have \(\bar{u}_{n}(k)=0\) for all \(|k|\geq r(n)\). By the definition of \(\mathcal{S}\) in 36 , this implies that \(\mathcal{S}\bar{u}_{n}(k)=0\) for all \((k,n)\in \mathcal{O}\).
We now claim that \(\bar{u}_{n+1}(k)=0\) for all \((k,n)\in \mathcal{O}\). By the form of \(\bar{u}\), it suffices to show that \[\label{steponebound46parta} r(n+1)\leq r(n)+1,\tag{39}\] since in this case, \(|k|\geq r(n)+1\geq r(n+1)\) implies \(\bar{u}_{n+1}(k)=0\).
To verify 39 , we use 35 and the fact that \(\beta\in (0,1)\), which implies that \[r(n+1)\leq r(n)+\max_{t\geq 0}\left|\frac{dr}{dt}\right|= r(n)+\max_{t\geq 0}\frac{R\beta}{T_{0}}\bigg(1+\frac{t}{T_{0}}\bigg)^{\beta-1}\leq r(n)+\frac{R\beta}{T_{0}}\leq r(n)+\frac{\Gamma^{m}}{2d\gamma R}.\] Since \(\Gamma\in (0, \frac{1}{3})\) and \(R \geq (2d\gamma)^{-1}\), this implies 39 , and hence \(\bar{u}_{n+1}(k)=0\) for all \((k,n)\in \mathcal{O}\). Combining this with the first observation, we obtain the desired result. ◻
The next result pertains to the total error in the gap.
Proposition 24. There exists \(c_{g}=c_{g}(d, m)>0\) such that for any \(\Gamma\in (0,1]\) and any \(R\geq 2\sqrt{d}\), for \(\mathcal{G}\) as defined in 38 and \(\mathcal{S}\) as defined in 36 , \[\sum_{(k,n)\in \mathcal{G}} (\bar{u}_{n+1}(k)-\mathcal{S}\bar{u}_{n}(k))_{+}\leq c_{g}\Gamma R^{d-\frac{1}{m}}.\]
In order to prove Proposition 24, we require some bounds on “how long” points spend in the region \(\mathcal{G}\). For \(k\in \mathbb{Z}^{d}\) such that \((k,n)\in \mathcal{G}\), we define \[\label{e46quantities} \begin{cases} \mathop{\rm duration}(k) = \#\{n: (k, n) \in \mathcal{G}\}=\text{``the number of steps that k is in the gap''.}\\ U(k) = \max\{\bar{u}(k, n) \vee \bar{u}(k, n+1): (k, n) \in \mathcal{G}\}. \end{cases}\tag{40}\] Observe that if \((k,n)\in \mathcal{G}\), then \(|k| \ge r(n) - \sqrt{d} \ge R - \sqrt{d} \ge R/2\) by the choice of \(R\), which implies that \[\label{e46Gbd} \left\{k: (k, n)\in \mathcal{G}\right\}\subset \left\{k: |k|>R/2\right\}.\tag{41}\]
We now estimate both of the quantities in 40 .
Lemma 25. There exists \(c_{u}=c_{u}(d,m)>0\) such that for any \(\Gamma\in (0,1]\), \(R\geq 2\sqrt{d}\), for all \(k\) with \((k,n)\in \mathcal{G}\), \[U(k)\leq c_{u}{R^d \,\Gamma \over |k|^{d+1/m}}\quad\text{and}\quad \mathop{\rm duration}(k) \,U^m(k) \le c.\]
Proof. Fix \(k\) such that \((k,n)\in \mathcal{G}\). We first prove that there exists a constant \(c=c(d,m)\) such that \[\label{durationestimate} \mathop{\rm duration}(k) \le c{|k|^{dm+1} \over R^{dm} \Gamma^m}.\tag{42}\] In order to estimate \(\mathop{\rm duration}(k)\), we consider the function \(h: [0, \infty)\rightarrow [0, \infty)\) defined by \(h(s):=r^{-1}(s)=T_{0}((s/R)^{1/\beta}-1)={T_0}((s/R)^{dm+2} - 1)\).
The function \(h\) is convex, and there exists \(c=c(d,m)>0\) such that \[h'(s) = {{T_0}\over \beta R^{\frac{1}{\beta}}} s^{dm+1}= {2d\gamma R^{2-\frac{1}{\beta}} s^{dm+1} \over \beta \Gamma^m}= c{s^{dm+1} \over R^{dm} \Gamma^m}>0.\] Set \(t_{1}:=h(|k|-1)\) and \(t_{2}:=h(|k|+\sqrt{d})\), and note that \(\left\{n: (k,n)\in \mathcal{G}\right\}\subset \left\{n: t_1<n\leq t_{2}\right\}\). By convexity and the derivative estimate above, we estimate \[\begin{align} t_{2}-t_{1}\leq h'(|k|+\sqrt{d})\Big[(|k|+\sqrt{d})-(|k|-1)\Big]\leq {c \over R^{dm} \Gamma^m} (|k| + \sqrt{d})^{dm+1}. \end{align}\] This implies that \[\mathop{\rm duration}(k)\leq {c \over R^{dm} \Gamma^m} (|k| + \sqrt{d})^{dm+1}+1.\] We have assumed that \(R\geq 2\sqrt{d}\), so by 41 , \(|k|\geq \sqrt{d}\). Moreover, since \(\Gamma \le 1\), we have \(|k|^{dm+1} (R^{dm} \Gamma^m)^{-1}\ge 2^{-dm}|k|\Gamma^{-m}\geq \sqrt{d}2^{-dm}\), and hence, by increasing \(c\), we obtain 42 .
We now fix \(n\in V(k) := \{n : (k,n) \in \mathcal{G} \text{ or } (k,n-1) \in \mathcal{G}\}\). As we show in 43 below, \(V(k)\) can be used to control \(U(k)\).
We introduce some more notation to simplify (35 ). Set \(\vartheta=\vartheta(k) := |k| / r(n)\), so that \[\bar{u}_n(k) = {R^d \, \Gamma \over r(n)^d} \left(1 - \vartheta^2\right)_+^{1/m},\] and \(\mathcal{G}=\left\{(k,n): \vartheta \in \big[1- \tfrac{\sqrt{d}}{r(n)}, 1+\tfrac{1}{r(n)}\big)\right\}\). For \((k, n)\in \mathcal{G}\) such that \(|k|\leq r(n)\), \[1-\vartheta^2 = (1+\vartheta)(1-\vartheta) \le 2(1-\vartheta)\leq 2 \frac{\sqrt{d}}{r(n)}=:\frac{c'}{r(n)}.\]
If \((k,n-1)\in \mathcal{G}\), then by (39 ) and the fact that \(d> 1\), we have \[|k| \ge r(n-1) - \sqrt{d} \ge r(n) - 1 - \sqrt{d}\geq r(n)-2\sqrt{d}.\] In this case, we obtain the identical estimate above that if \(|k|\leq r(n)\), \[1-\vartheta^2\leq 2(1-\vartheta)\leq 2\frac{2\sqrt{d}}{r(n)}\leq \frac{2c'}{r(n)}.\]
Therefore, for \((k, n)\in \mathcal{G}\) or \((k, n-1)\in \mathcal{G}\) such that \(|k|\leq r(n)\), we have \[\bar{u}_n(k)={R^d\,\Gamma\over r(n)^d}\left(1-\vartheta^2\right)^{1/m} \le 2c'{R^d\,\Gamma \over r(n)^{d+1/m}} \le 2c'{R^d \, \Gamma \over |k|^{d+1/m}}.\] If \(|k|>r(n)\), then \(\bar{u}_n(k) = 0\) and the same inequality holds. Therefore, for \(k\) such that \((k, n)\in \mathcal{G}\), \[\label{estimateforu} U(k) = \max\{\bar{u}_{n}(k) \vee \bar{u}_{n+1}(k): (k, n) \in \mathcal{G}\}=\max_{n\in V(k)} \bar{u}_{n}(k)\le 2c'{R^d \,\Gamma \over |k|^{d+1/m}}.\tag{43}\] Combining this with (42 ), we obtain the existence of \(c_{u}=c_{u}(d,m)>0\) such that \[\label{durationanduestimate}\mathop{\rm duration}(k) \,U^m(k) \le c_{u}.\tag{44}\] ◻
Equipped with Lemma 42 , we may now prove Proposition 24.
Proof of Proposition 24. Fix \(k\) such that \((k,n)\in \mathcal{G}\). Then from (37 ), dropping negative terms from the right hand side, and then taking the positive part, we obtain \[(\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_{+} \le (\bar{u}_{n+1}(k) - \bar{u}_n(k))_{+} + \bar{u}_{n}(k)^{m+1}.\] Since \(r(t)\) is monotone, by the definition of \(\mathcal{G}\), \(\left\{n: (k,n)\in \mathcal{G}\right\}\) is a discrete interval. Moreover, since \(t\mapsto \bar{u}(k,t)\) is unimodal in \(t\) by Lemma 11(i), it follows that \(E:=\left\{n: \bar{u}_{n+1}(k)-\bar{u}_{n}(k)>0\right\}\) is also a discrete interval. Therefore, \[\begin{align} \sum_{n: (k,n) \in \mathcal{G}} (\bar{u}_{n+1}(k) - \bar{u}_{n}(k))_{+}\leq \sum_{n\in E: (k,n)\in \mathcal{G}} (\bar{u}_{n+1}(k) - \bar{u}_{n}(k)) \le \max_{n: (k,n) \in \mathcal{G}}\bar{u} (k, n+1)\le U(k), \end{align}\] where we used that the sum telescopes, and that \(\bar{u}\geq 0\) everywhere. By Lemma 25, this implies that there exists \(c=c(d,m)\) such that \[\begin{align} \sum_{n: (k,n) \in \mathcal{G}} (\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_{+} &\le U(k)+\sum_{n: (k,n) \in \mathcal{G}} \bar{u}_{n}(k)^{m+1}\\ &\leq U(k)+\mathop{\rm duration}(k)U(k)^{m+1}\\ &\leq cU(k). \end{align}\] Combining this with Lemma 25 and 41 , we obtain that \[\label{gaperrorfinal} \begin{align} \sum_{(k,n)\in \mathcal{G}} (\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_{+} &\leq \sum_{k\in \mathbb{Z}^d:|k| \ge R/2} cU(k)\\ &\le cR^d\,\Gamma \sum_{k\in \mathbb{Z}^d: |k| \ge R/2} \frac{1}{|k|^{d+1/m}} \\&\le cR^d \,\Gamma \int_{R/2}^{\infty} \frac{r^{d-1}}{r^{d+1/m}}\, dr=:c_{g}\Gamma R^{d-\frac{1}{m}}, \end{align}\tag{45}\] where \(c_{g}=c_{g}(d,m)\). ◻
The final preliminary result concerns the core region.
Proposition 26. There exists \(c_{c}=c_{c}(d,m)>0\) such that for any \(\Gamma>0\), \(R>0\), for \(\mathcal{C}\) as defined in 38 and \(\mathcal{S}\) as defined in 36 , \[\sum_{(k,n)\in \mathcal{C}} (\bar{u}_{n+1}(k)-\mathcal{S}\bar{u}_{n}(k))_{+}\leq c_{c}R^{d-2} \,\Gamma^{m+1}.\]
In the core region, we know that the continuous function \(\bar{u}\) solves the porous medium equation \(\partial_t \bar{u} = {1 \over 2d} \Delta(\bar{u}^{m+1})\). By (37 ) this implies \[\begin{align} \bar{u}_{n+1}(k) - \mathcal{S}\bar{u}(k, t)&= \underbrace{\bar{u}(k, n+1) - \bar{u}(k, n) - {\partial \bar{u} \over \partial t}(k,n)}_{\text{(time error)}}\\ &\quad+\underbrace{{1 \over 2d} \Delta (\bar{u}^{m+1}(k,n)) - {1 \over 2d} \sum_{\ell\sim k} [\bar{u}(\ell, n)^{m+1} - \bar{u}(k, n)^{m+1}]}_{\text{(space error)}}. \end{align}\]
We now estimate the contributions of these two error terms individually. Proposition 26 is an immediate consequence of the following two lemmas.
Lemma 27. There exists \(c_{c}=c_{c}(d,m)>0\) such that for any \(\Gamma>0\) and \(R>0\), for \(\mathcal{C}\) as defined in 38 , \[\sum_{(k,n)\in \mathcal{C}}\left(\bar{u}(k, n+1) - \bar{u}(k, n) - {\partial \bar{u} \over \partial t}(k,n)\right)_{+}\leq c_{c}R^{d-2} \,\Gamma^{m+1}.\]
Lemma 28. For \(\mathcal{C}\) as defined in 38 , \[\sum_{(k,n)\in \mathcal{C}}\left({1 \over 2d} \Delta (\bar{u}^{m+1}(k,n)) - {1 \over 2d} \sum_{\ell\sim k} [\bar{u}(\ell, n)^{m+1} - \bar{u}(k, n)^{m+1}]\right)_{+}=0.\]
Proof of Lemma 27. As a consequence of Taylor’s theorem, there exists \(s\in [n, n+1]\) such that \[\bar{u}(k, n+1) - \bar{u}(k, n) - \partial_t \bar{u}(k, n) = \frac{1}{2} \partial^2_t \bar{u}(k, s),\] and thus, we will be concerned with estimating \(\left(\partial^2_t \bar{u}(k, t)\right)_{+}\). Recall the parameterization \(\vartheta=\vartheta(x,t)=|x| / r(t)\); that in Lemma 11(ii), we computed \(\partial_{t}\bar{u}\) in 24 ; and that \(\tfrac{\partial \vartheta}{\partial t} =- \tfrac{\vartheta\beta}{(t + {T_0})}\). Thus, by a direct computation, we have that \[\label{eq:partial2t} \partial^{2}_{t}\bar{u}(x, t) = {R^d\Gamma(1 - \vartheta^2)^{\tfrac{1}{m}}\over r(t)^d m(t+T_0)^2} \left[-\left({2\beta \over 1 - \vartheta^2} - 1\right) + {1 \over m} \left({2\beta \over 1 - \vartheta^2} - 1\right)^2 - {4\beta^2 \vartheta^2 \over (1 - \vartheta^2)^2}\right],\tag{46}\] and combining terms, it follows that there exist positive constants \(K_{1}, K_{2}\), and \(K\), depending only on \(d,m\), such that \[\begin{align} \label{gbound} \partial^{2}_{t} \bar{u}(x, t)&\leq {R^d\Gamma\over r(t)^d m(t+T_0)^2}\left[K_{1} (1 - \vartheta^2)^{\tfrac{1}{m}} + K_2(1 - \vartheta^2)^{\tfrac{1}{m} - 1} + 4\beta^2 (\tfrac{1}{m} - \vartheta^2) (1 - \vartheta^2)^{\tfrac{1}{m}-2}\right]\notag\\ &\leq {KR^d\Gamma\over r(t)^d m(t+T_0)^2}(1 - \vartheta^2)^{\tfrac{1}{m} - 1}\notag\\&={KR^d\Gamma\over r(t)^d m(t+T_0)^2}\bigg(1 - \Big(\frac{|x|}{r(t)}\Big)^{2}\bigg)^{\tfrac{1}{m} - 1}=: g(x,t), \end{align}\tag{47}\] where for the last inequality, we used that \(m\geq 1\). We now simply need to obtain an upper bound on the function \(g\). First, since \(m\geq 1\), \(t\mapsto g(k,t)\) is a decreasing function, and hence by the first observation of the proof, \[\label{e46taylors} \bar{u}(k, n+1) - \bar{u}(k, n) - \partial_t \bar{u}(k, n)\leq \frac{1}{2}g(k,n).\tag{48}\] Furthermore, by definition of \(g\), it is clear that \(g\geq 0\) on \(\mathcal{C}\) and that for any \(t\) fixed, \(g(k,t)\) is monotone increasing with respect to \(|k|\) in \(\mathcal{C}\).
Fix \(n\) such that there exists \(k\) with \((k,n)\in \mathcal{C}\). We claim that \[\label{e46core1} \sum_{k: (k,n)\in \mathcal{C}} g(k,n) \le \int\limits_{B_{r(n)}} g(y, n) \,dy,\tag{49}\] where \(B_{r(n)}\) is the Euclidean ball in \(\mathbb{R}^{d}\) of radius \(r(n)\). In order to prove 49 , due to the symmetry of \(g\), it is enough to prove an analogous bound in the positive orthant \(E_{n}^{+}:=\mathbb{Z}^{d}_{+}\cap \left\{k: (k,n)\in \mathcal{C}\right\}\). More precisely, since \(k\in E_{n}^{+}\), we know \(|k| < r(n) - \sqrt{d}\), and hence \([k_{1}, k_{1}+1]\times \ldots [k_{d}, k_{d}+1]\subseteq \left\{|k|<r(n)\right\}=B_{r(n)}\cap \mathbb{Z}^{d}\). Owing to the monotonicity property of \(g\), we conclude \[\sum_{k\in E_{n}^{+}} g(k,n) \le \int_{\bigcup_{k\in E_{n}^{+}} [k_{1}, k_{1}+1]\times \ldots [k_{d}, k_{d+1}]}g(y,n) \,dy \le \int\limits_{\mathbb{R}^{d}_{+}\cap B_{r(n)}} g(y,n) \,dy,\] where \(\mathbb{R}^d_+ = [0, \infty)^d\). Summing over all orthants, we obtain 49 .
We now conclude by 49 that \[\begin{align} \sum_{k: (k,n)\in \mathcal{C}} g(k,n) &\leq {K R^d \Gamma \over r(n)^d(n+T_0)^2} \int_{B_{r(n)}} \Big(1 - \frac{|y|^{2}}{r(n)^{2}}\Big)^{\tfrac{1}{m}-1} \,dy \\&= {K R^d \Gamma \over (n+T_0)^2} \int_{B_{1}} (1 - z^2)^{\tfrac{1}{m}-1} \,dz \\&= {KR^d \,\Gamma \over (n+T_0)^2}, \end{align}\] by increasing the value of \(K=K(d,m)\) if necessary.
Combining this with 48 and repeatedly adjusting the constant \(K\) as needed, we obtain \[\sum_{(k,n)\in \mathcal{C}}\left(\bar{u}(k, n+1) - \bar{u}(k, n) - {\partial \bar{u} \over \partial t}(k,n)\right)_{+}\le \sum_{n=0}^\infty {KR^d \Gamma \over (n+T_0)^2} \le {KR^d \Gamma \over T_0}=KR^{d-2} \,\Gamma^{m+1},\] where we used the definition of \(T_{0}\) from 35 . The result follows. ◻
Proof of Lemma 28. For fixed \((k,n)\in \mathcal{C}\), we can re-express the space error as \[{1 \over 2d} \Delta(\bar{u}(k,n))^{m+1}- {1 \over 2d} \sum_{\ell\sim k} [\bar{u}(\ell, n)^{m+1} - \bar{u}(k,n)^{m+1}] = \sum_{i=1}^d \mathcal{E}_i(k, n)\] where \(\mathcal{E}_i\) is the error along a single coordinate: \[\mathcal{E}_i(k,n) := {1 \over 2d} \left[{\partial^2 \over \partial^2 x_i} \bar{u}(k, n)^{m+1} - \left(\bar{u}(k+e_i, n)^{m+1} - 2\bar{u}(k, n)^{m+1} + \bar{u}(k-e_i, n)^{m+1}\right)\right] .\]
To estimate the error, we observe the following: if \(f \in C^4(\mathbb{R})\), then \[\label{e46ibp} f''(x) - (f(x+1) - 2f(x) + f(x-1)) = -\int_{x-1}^{x+1} {(1 - |s-x|)^3 \over 6} f^{(4)}(s) \,ds.\tag{50}\] The proof of 50 relies on the integral version of Taylor’s theorem, and appears immediately after this argument.
Using 50 , we obtain the alternative formula \[\mathcal{E}_i(k,n) = -{1\over2d} \int_{k_i - 1}^{k_i + 1} {(1 - |s - k_i|)^3 \over 6} \partial^4_i(\bar{u}^{m+1}(k_1, \ldots, k_{i-1}, s, k_{i+1}, \ldots, k_d)) \,ds. \label{errori}\tag{51}\] By Lemma 11(ii), \(\bar{u}^{(4)}(k,n)\geq 0\) for all \((k,n)\in \mathcal{C}\). This completes the proof. ◻
Proof of 50 . By Taylor’s theorem in integral form, we have \[\begin{align} f(x+1)&=f(x)+f'(x)+\frac{1}{2}f''(x)+\frac{1}{6}f^{(3)}(x)+\int_{x}^{x+1}f^{(4)}(s)\frac{(1-|s-x|)^{3}}{6}\, ds,\\ f(x-1)&=f(x)-f'(x)+\frac{1}{2}f''(x)-\frac{1}{6}f^{(3)}(x)+\int_{x-1}^{x}f^{(4)}(s)\frac{(1-|s-x|)^{3}}{6}\, ds. \end{align}\] Adding the two expressions and rearranging, we arrive at 50 . ◻
In order to conclude, we require one additional result to control \(\mathop{\rm smallest}(\bar{u})\).
Lemma 29. There is a constant \(c_0 = c_0(d,m)>0\) such that for any \(\Gamma\in (0,1]\) and \(R\geq 2\sqrt{d}\), \(\mathop{\rm smallest}(\bar{u}) \ge c_0R^d \Gamma\).
Proof. According to the form of the Barenblatt solution, as previously noted, at a fixed time \(n\), \(\bar{u}_n(k)\) decreases as \(|k|\) increases. Consequently, if \(k\in\mathbb{Z}^{d}_{+}\), \[\bar{u}_n(k) \ge \int_{[k_1,k_1+1] \times \cdots[k_d,k_d+1]} \bar{u}_{n}(x) \,dx.\] This implies that \[|\bar{u}_n |_1 = \sum_{k\in \mathbb{Z}^d} \bar{u}_n(k) \ge \sum_{k\in \mathbb{Z}^{d}_{+}} \bar{u}_{n}(k)\geq \int_{[1, \infty)^d} \bar{u}_{n}(x)\, dx.\]
Using 35 and a change of variables, with \(B_{r(n)}\) denoting the Euclidean ball of radius \(r(n)\), we have \[\begin{align} \int_{[1, \infty)^{d}} \bar{u}_n(x) \,dx &= {R^d \Gamma \over r(n)^d} \int\limits_{[1, \infty)^{d}\cap B_{r(n)}} \left(1 - \left({|x| \over r(n)}\right)^2\right)^{1/m} \,dx \\&= R^d \Gamma \int\limits_{[r(n)^{-1}, \infty)^{d}\cap B_{1}} (1-|y|^2)^{1/m} \,dy. \end{align}\]
Since \(R = r(0) \geq 2 \sqrt{d}\), it follows that for every \(n\geq 0\), \([r(n)^{-1}, \infty)^{d}\supseteq [(2\sqrt{d})^{-1}, \infty)^{d}\). Thus \[\int_{[1, \infty)^{d}} \bar{u}_n(x) \ge R^d \Gamma \int\limits_{[(2\sqrt{d})^{-1}, \infty)^{d}\cap B_{1}} (1-|y|^2)^{1/m} \,dy=: c_{0}R^{d} \Gamma.\] It is clear that \(c_{0}=c_{0}(d,m)>0\), and hence \(|\bar{u}_n|_1=\sum_{k} \bar{u}_n(k) \ge c_0 R^d \Gamma\). Since \(n\) was arbitrary, the result follows. 0◻
Proof of Proposition 22. We now make explicit choices of \(R\) and \(\Gamma\). We allow arbitrarily small \(\Gamma\in (0,\frac{1}{3})\), while \(R\in [1, \infty)\) will be moderately large and fixed, given by \[\label{e46Rdef} R = \max\left\{2\sqrt{d}, (2d\gamma)^{-1}, \left( 4c_g\over c_0\right)^{m}, \sqrt{\frac{4c_c}{c_{0}}}\right\},\tag{52}\] where the constant \(c_0\) is from Lemma 29, \(c_g\) is from Proposition 24, and \(c_c\) is from Proposition 26. All these constants (and hence \(R\) itself) depend only on \(d\) and \(m\).
Choosing \(R\) as in 52 and \(\Gamma<1/3\), the hypotheses of Proposition 23, Proposition 24 and Proposition 26 hold simultaneously. It follows that \[\begin{align} \sum_{(k,n)\in \mathbb{Z}^{d}\times {\mathbb{N}}}& (\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_+\\ &\leq \sum_{(k,n)\in \mathcal{O}}(\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_+ +\sum_{(k,n)\in \mathcal{G}}(\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_+\\ &\quad +\sum_{(k,n)\in \mathcal{C}}(\bar{u}_{n+1}(k) - \mathcal{S}\bar{u}_n(k))_+\\ &\leq c_{g}\Gamma R^{d-\frac{1}{m}}+c_{c}R^{d-2} \,\Gamma^{m+1}. \end{align}\] To bound each of these terms, we will use Lemma 29 which says \(\mathop{\rm smallest}(\bar{u})\geq c_0 R^d \Gamma\).
For the first term, by the choice of \(R\), \(R \ge \left(\tfrac{4c_g}{c_{0}}\right)^{m}\), so \[c_{g}\Gamma R^{d-\frac{1}{m}}\leq c_{g}\Gamma R^{d}\frac{c_{0}}{4c_{g}}\leq \frac{1}{4}\mathop{\rm smallest}(\bar{u}).\]
Similarly, for the second term, by choice of \(R\), \(R^{2}\geq 4c_{c}c_{0}^{-1}\). Hence \[c_{c}R^{d-2} \,\Gamma^{m+1}\leq \frac{c_{0}}{4}R^{d}\Gamma^{m+1}\leq \frac{1}{4}\Gamma^{m}\mathop{\rm smallest}(\bar{u})\leq \frac{1}{4} \mathop{\rm smallest}(\bar{u}).\] This yields the desired claim. ◻
We now recall the function \((\tilde{p}_{n})_{n\geq 0}\) defined in Lemma 19, which is a solution of 14 on \([0, \infty)\) with initial condition \(\tilde{p}_{0}\), where \(\tilde{p}_n(k)\in [0, \frac{1}{3}]\) is volcanic for all \(n\). Moreover, by definition of the scheme, \(\tilde{p}_n(k)\) is strictly positive whenever \(|k|_1 \le n\).
We aim to control \(\mathrm{dist}[\bar{u}_{n}, \tilde{p}_{n+n_{0}}]\) for some \(n_{0}\in \mathbb{N}\) to be chosen. Since \((\tilde{p}_{n+n_{0}})_{n\geq 0}\) is still a solution of the scheme 14 on \([0, \infty)\) with initial condition \(\tilde{p}_{n_{0}}\), as a consequence of Proposition 22 and Lemma 21, for any \(\Gamma\in (0, \frac{1}{3})\) and for a fixed \(R=R(d,m)\), for \(\bar{u}=\bar{u}^{(R, \Gamma)}\), we have \[\mathrm{dist}[\bar{u}_{n}, \tilde{p}_{n+n_{0}}]\leq \mathrm{dist}[\bar{u}_{0}, \tilde{p}_{n_{0}}]+\frac{1}{2}\mathop{\rm smallest}(\bar{u}).\]
We now choose \(n_{0}\) (and \(\Gamma\)) so that \(\mathrm{dist}[\bar{u}_{0}, \tilde{p}_{n_{0}}]=0\). Set \[\label{e46n0ga} n_0 = \lceil R \sqrt{d} \rceil\quad\text{and}\quad \Gamma = (\min_{|k| \le R} \tilde{p}_{n_0}(k))\wedge \frac{1}{3}.\tag{53}\] Observe that both \(n_{0}\) and \(\Gamma\) depend only on \(d,m\), since \(R=R(d,m)\). Recall that \(\|\bar{u}\|_{L^{\infty}(\mathbb{R}^{d}\times [0, \infty))}\leq \Gamma\), and \(R<n_{0}\), we know \(\Gamma>0\). Letting \(\bar{u}_{n}=\bar{u}^{(R,\Gamma)}(\cdot, n)\) for these choices of \(R, \Gamma\), we have \[\mathrm{dist}[\bar{u}_{0}, \tilde{p}_{n_{0}}]=\sum_{k\in \mathbb{Z}^{d}} \left(\bar{u}_{0}(k)-\tilde{p}_{n_{0}}(k)\right)_{+}\leq \sum_{|k| \le R} (\Gamma - \tilde{p}_{n_0}(k))_+ = 0.\] Combining this with the prior display, we have that for these choices of \(n_{0}, \Gamma, R\), \[\label{e46intermed} \mathrm{dist}[\bar{u}_{n}, \tilde{p}_{n+n_{0}}]=\sum_{k\in \mathbb{Z}^{d}} \left(\bar{u}_{n}(k)-\tilde{p}_{n+n_{0}}(k)\right)_{+}\leq \frac{1}{2}\mathop{\rm smallest}(\bar{u}).\tag{54}\]
This observation now allows us to prove the following lower bound on \(\tilde{p}\) inside the support of the associated Barenblatt solution \(\bar{u}\).
Lemma 30. Let \(R\) be defined as in 52 and \(n_{0}, \Gamma\) be defined by 53 , which only depend on \(d,m\). There are positive constants \(c=c(d, m)<1\) and \(N=N(d,m)\) such that for all \(n\geq N\), \[\tilde{p}_{n+n_0}(k) \ge \frac{c}{r(n)^d} \quad\text{for all |k|\leq cr(n).}\]
Proof. Let \(g(z) := R^d \Gamma (1 - |z|^2)^{1/m}_+\), and note that \(\int_{\mathbb{R}^{d}} g(z)\, dz>0\). We consider the set \(A(c) = \{z \in \mathbb{R}^d: |z_1|, \ldots, |z_d| \ge c\}\) which is simply the complement of the ball of radius \(c\) in the \(L^{\infty}\)-norm. As \(c \to 0+\), as a consequence of the monotone convergence theorem, we have \[\lim_{c \to 0+} \int_{A(c)} (g(z) - c)_+ \,dz = \int_{\mathbb{R}^d} g(z) \,dz.\] Consequently, we may fix a constant \(c=c(d,m)\in (0,1)\) such that \[\label{e46c3choice} \int_{A(c)} (g(z) - c)_+ \,dz \ge \frac{2}{3} \int_{\mathbb{R}^d} g(z) \,dz.\tag{55}\]
Let \(A_n(c) := \{k\in \mathbb{Z}^d: |k_1|, \ldots, |k_d| \ge cr(n)\}\). Recall that by Lemma 19, \(\tilde{p}_{n+n_{0}}\) is volcanic for every \(n\). It follows (by applying the volcanic property iteratively over neighbors) that for any \(k\in A_{n}(c)\) and \(\ell\in \mathbb{Z}^{d}\) with \(|\ell| \le cr(n)\), \(\tilde{p}_{n+n_{0}}(k) \le \tilde{p}_{n+n_{0}}(\ell)\). Therefore, by 54 , for any fixed \(|\ell| \le cr(n)\), \[\label{lowerboundonp46one} \sum_{k\in A_{n}(c)} \left(\bar{u}_{n}(k)-\tilde{p}_{n+n_{0}}(\ell)\right)_{+}\leq \sum_{k\in \mathbb{Z}^{d}} \left(\bar{u}_{n}(k)-\tilde{p}_{n+n_{0}}(k)\right)_{+}\leq \frac{1}{2}\mathop{\rm smallest}(\bar{u})\leq \frac{1}{2}|\bar{u}_{n}|_{1}.\tag{56}\]
By definition of \(\bar{u}_{n}\) in 35 \[\label{e46grel} \bar{u}_n(r(n)z) = {R^d \Gamma \over r(n)^d} \left(1 - |z|^2\right)^{1/m}_+ = \frac{g(z)}{r(n)^{d}}.\tag{57}\] Since \(r(n)\to \infty\) as \(n\to \infty\), we may apply a Riemann approximation to conclude that \[\lim_{n \to \infty} |\bar{u}_n |_1= \lim_{n \to \infty} \frac{1}{r(n)^{d}} \sum_{ (r(n)z)\in \mathbb{Z}^{d}} g(z) = \int_{\mathbb{R}^d} g(z) \,dz.\] As another consequence of 57 , we have \[\begin{align} \lim_{n \to \infty} \sum_{k\in A_n(c)} \left(\bar{u}_n(k) - \frac{c}{r(n)^d}\right)_+ = \lim_{n \to \infty} \frac{1}{r(n)^{d}} \sum_{r(n)z \in A_n(c)} (g(z) - c)_+ = \int_{A(c)} (g(z) - c)_+ \,dz. \end{align}\] By 55 and the prior display, we have \[\lim_{n \to \infty} \sum_{k\in A_n(c)} \left(\bar{u}_n(k) - \frac{c}{r(n)^d}\right)_+\geq \lim_{n \to \infty} \frac{2}{3}|\bar{u}_n |_1>0.\] Consequently, there is \(N>0\) so that for all \(n \ge N\), \[\sum_{k\in A_n(c)} \left(\bar{u}_n(k) - \frac{c}{r(n)^d}\right)_+\geq \frac{5}{9}|\bar{u}_n |_1>0.\] Now for the purposes of contradiction, fix \(n \ge N\), and suppose that there is a point \(\ell\) such that \(|\ell| \le cr(n)\) and \(\tilde{p}_{n+n_{0}}(\ell) < \tfrac{c}{r(n)^d}\). Then by the prior display, \[\sum_{k\in A_n(c)} (\bar{u}_n(k) - \tilde{p}_{n+n_{0}}(\ell))_+ \ge \sum_{k\in A_n(c)} \left(\bar{u}_n(k) - \frac{c}{r(n)^d}\right)_+ \ge \frac{5}{9} |\bar{u}_n |_1,\] which contradicts the inequality (56 ). This implies that \(\tilde{p}_{n+n_{0}}(k) \ge \tfrac{c}{r(n)^d}\) if \(|k| \le cr(n)\) and \(n \ge N\). ◻
Equipped with Lemma 30, we are now ready to finish the proof of Theorem 2(i).
Proof of Theorem 2(i). By Lemma 30, for \(n_{0}\) as in 53 , and by the definition of \(r\) in 35 , by adjusting \(c=c(d,m)\), we have that for all \(n\geq N\), \[\tilde{p}_{n+n_0}(k) \ge \frac{c}{r(n)^d}=\frac{c}{(T_{0}+n)^{d\beta}} \quad\text{for all |k|\leq cr(n).}\] Consequently, for all \(n\geq N\vee T_{0}\), by adjusting \(c=c(d,m)\) and since \(n_{0}>0\), we have \[\tilde{p}_{n+n_0}(k) \ge \frac{c}{(2n)^{d\beta}}\geq \frac{c}{(n+n_{0})^{d\beta}}.\] By Theorem 12, it follows that for all \(n\geq n_{0}+ (N\vee T_{0})\), \(\sup_{k} \tilde{p}(k,n)\leq C'n^{-d\beta}\). For \(N_{0}\) as in Lemma 19, this implies that there is \(C''=C''(d,m)\) such that for all \(n\geq n_{0}+ N\vee T_{0}\), we have \[p(k,n+N_{0})\leq \tilde{p}(k,n)\leq C'n^{-d\beta}\leq C''(n+N_{0})^{-d\beta}\quad\text{for all k\in \mathbb{Z}^{d}.}\] Since \(n_{0}, N_{0}, N, T_{0}\) all depend only on \(d,m\) and are all finite, this statement can then be upgraded to the statement that there exists \(C=C(d,m)>0\) such that \[p(k,n)\leq Cn^{-d\beta}\quad\text{for all n\in \mathbb{N} and all k\in \mathbb{Z}^{d}.} \qedhere\] ◻
In this section, we prove Theorem 2(ii) and Theorem 2(iii).
We prove that there is a constant \(C=C(d,m)>0\) such that for all \(r > 0\) and \(n \in {\mathbb{N}}\), \[\sum_{k\in \mathbb{Z}^{d}\cap B^{c}_{rn^{\beta}}} p(k,n)= \sum_{|k|>rn^{\beta}}p(k,n)\leq C \exp(-r/C).\] We begin by recalling Freedman’s inequality, which is a type of concentration inequality. Let \((\mathscr F_n)_{n\geq 0}\) be a filtration and \(Y_n\) be a real-valued martingale with \(Y_0 = 0\). Let \(V_n:=\text{Var}[Y_n \mid \mathscr F_{n-1}]\) be the conditional variance.
Theorem 31. [17] If \(|Y_{n+1} - Y_n| \le 1\) for all \(n\), then for any \(a, b>0\), \[\mathbb{P}\left(\exists n: Y_n \ge a \text{ and } \sum_{j=1}^n V_j \le b\right) \le \exp\left(-{a^2 \over 2(a+b)}\right).\]
Equipped with this result, we can now proceed with the proof of Theorem 2(ii).
Proof of Theorem 2(ii). If \(r\in (0,1]\), we obtain the desired bound for all \(n\in \mathbb{N}\), so long as \(C>1.\) Thus, let \(r > 1\), and let \((X_j)_{j\in \mathbb{N}}\) be \(\text{CM}(m)\)-distributed. Fix \(i \in [d]\), and let \(Y_j\) be the \(i\)-th coordinate of \(X_j\).
At any step of the \(\text{CM}(m)\), with probability \(p^m / d\), we move in the \(i\)-th coordinate, and when we do, we take a Bernoulli step that is conditionally independent of the past. Thus, \((Y_j)_{j\geq 0}\) is a martingale, and its conditional variance is given by \[V_{j}=\text{Var}[Y_j \mid \mathscr F_{j-1}] = \mathbb{E}[(Y_j - Y_{j-1})^2 \mid \mathscr F_{j-1}] = \frac{1}{d}p^m(X_{j-1}, j-1).\]
By Theorem 2(i), this has a deterministic upper bound, given by \[V_j = c p^m(X_{j-1}, j-1) \le {c \over j^{dm\beta}}.\] Since \(0 < dm\beta < 1\), we have \[\sum_{j=1}^{n}V_{j}=c\sum_{j=1}^n j^{-dm\beta} = cn^{1-dm\beta} + O(1),\] which implies \(\sum_{j=1}^n V_j \le cn^{1-dm\beta} = Cn^{2\beta}\), where \(C=C(d,m)\). Let \(b:=Cn^{2\beta}\), so that \(\sum_{j=1}^n V_j \le b\).
Let \(a:=rn^\beta/\sqrt{d}\). Then by properties of norm-equivalences on \(\mathbb{R}^{d}\), we have \[\{|X_n| \ge rn^\beta\} \subseteq \bigcup_{i=1}^d\{(X_n)_i \ge a\} \cup \bigcup_{i=1}^d \{-(X_n)_i \ge a\}.\] By a union bound, symmetry of the process, and the prior claim, this implies \[\mathbb{P}\left(|X_n| \ge rn^\beta\right) \le 2d\mathbb{P}\left((X_n)_i \ge a\right) = 2d \mathbb{P}\left(Y_n \ge a\right) = 2d \mathbb{P}\left(Y_n \ge a \text{ and }\sum_{j=1}^n V_j \le b\right).\] We now conclude by using Freedman’s inequality (Theorem 31). In particular, we have \[\mathbb{P}\left(|X_n| \ge rn^\beta\right) \le 2d\mathbb{P}\left(Y_n \ge a \text{ and } \sum_{j=1}^n V_j \le b\right) \le 2d\exp\left(-{r^2 n^{2\beta}/d \over 2(rn^{\beta}/\sqrt{d} + Cn^{2\beta})}\right).\] Using that \(r > 1\), we conclude with the lower bound \[{r^2 n^{2\beta}/d \over 2(rn^{\beta}/\sqrt{d} + Cn^{2\beta})} = \frac{r^2}{2d(rn^{-\beta}/\sqrt{d} + C)} \geq \frac{r^2}{2d(r/\sqrt{d} + C)} \geq \frac{r^2}{C(r+1)} \geq \frac{r}{C}.\] ◻
The goal is to obtain an upper bound on the total variation of \(p(\cdot, n)\) for a domain \(D:=B_{rn^{\beta}}\cap\mathbb{Z}^{d}\) of the form \[[p(\cdot, n)]_{\mathop{\mathrm{TV}}(D)} := \frac{1}{2}\sum_{\{u,v\in D:u\sim v\}} |p(v,n)-p(u,n)|\leq Cr^{d-1}n^{-\beta}.\]
In order to prove this, we begin by introducing a weaker version of spatial monotonicity. We say that a function \(q: \mathbb{Z}^d \to \mathbb{R}\) is almost-volcanic if, \(q\) is symmetric, as in 19 , and for any two neighbours \(k\sim \ell\),
if \(|k|_1 > |\ell|_1 \ge 1\), then \(q(k) \le q(\ell)\), and if
if \(|k|_1 \ge 2\), then \(q(k) \le q(0)\).
Observe that this definition differs from the definition of volcanic by only requiring that \(q(\ell)\) is nondecreasing towards the origin for points \(|\ell|_{1}\geq 1\), and furthermore that \(q(0)\geq q(k)\) for \(|k|_{1}\geq 2\). We first show that being almost-volcanic is preserved under certain monotonicity conditions on the scheme. Unlike Lemma 9, the analogous statement for volcanic functions, we state this result directly for the specific function \(p_{n}\), the distribution of a (\(m\))-distributed process at time \(n\).
Lemma 32. For any \(n\in \mathbb{N}_{0}\), if \(0\leq p_{n}\leq 1/3\) is almost-volcanic, then \(p_{n+1}\) is almost-volcanic.
Proof. Recall that \(p=(p_{n})_{n\geq 0}\) solves the scheme 14 on \([0, \infty)\) with initial condition \(p_{0}=\mathbf{1}_{0}\), and by hypothesis, let us assume that \(0\leq p_{n}\leq 1/3\). Since \(A(u)=u^{m+1}\) in the scheme 14 , we have \(0\leq A'(\cdot)\leq \frac{2}{3}\) for \(0\leq u\leq \frac{1}{3}\).
By the same reasoning as in Lemma 9, if \(p_{n}\) is symmetric, then \(p_{n+1}\) is also symmetric. Therefore, it remains to verify that \(p_{n+1}\) satisfies the above two additional conditions necessary to be almost-volcanic.
We begin with the first claim, which is that \(p_{n+1}(k) \le p_{n+1}(\ell)\) for \(|k|_1 > |\ell|_1 \ge 1\). In the case of \(k, \ell\) with \(|\ell|_1 \ge 2\), this follows immediately from Case 1 in the proof of Lemma 9. Therefore, we simply need to check this inequality in the case when \(|k|_1 = 2, |\ell|_1 = 1\).
Suppose \(k\) is a point with \(|k|_1 = 2\). By symmetry, it is enough to consider the cases \(k= 2e_1\) or \(k= e_1 + e_2\).
Case 1. \(k= 2e_1\). If we look at all neighbors of \(e_1\), there are \(2d-2\) neighbours the form \(e_1 \pm e_j, j \ne 1\), one neighbor which is \(2e_{1}\) and one neighbor which is the origin. Thus, for \(\ell\sim e_{1}\), since \(p_{n}\) is almost-volcanic, the symmetry and monotonicity properties imply that \[p_{n}(\ell)\begin{cases} =p_n(e_1+e_2)&\text{if \ell=e_1 \pm e_j, j \ne 1},\\ =p_{n}(2e_{1})&\text{if \ell=2e_{1}},\\ \geq p_{n}(2e_{1})&\text{if \ell=0}. \end{cases}\] Therefore, since \(A\) is nondecreasing, we have \[\begin{align} p_{n+1}(e_1) &= p_n(e_1) + {1 \over 2d} \sum_{\ell\sim e_1} (A(p_n(\ell)) - A(p_n(e_1))) \\&\ge p_{n}(e_{1}) + {2d-2 \over 2d} (A(p_n(e_1+e_2)) - A(p_{n}(e_{1}))) + {2 \over 2d} (A(p_{n}(2e_{1})) - A(p_{n}(e_{1}))). \end{align}\]
On the other hand, \(2e_1\) has \(2d-2\) neighbours \(2e_1 \pm e_j, j \ne 1\), one neighbour that is \(e_1\), and one neighbour that is \(3e_1\). Using again the almost-volcanicity, we conclude \[p_{n}(\ell)\begin{cases} \leq p_n(e_1+e_2)&\text{if \ell=2e_1 \pm e_j, j \ne 1},\\ \leq p_{n}(2e_{1})&\text{if \ell=3e_{1}},\\ =p_{n}(e_{1})&\text{if \ell=e_{1}}. \end{cases}\]
Using the above and the scheme, we have that \[p_{n+1}(2e_1) \le p_{n}(2e_{1}) + {2d-2 \over 2d} (A(p_{n}(e_{1}+e_{2})) - A(p_{n}(2e_{1}))) + {1 \over 2d} (A(p_{n}(e_{1})) - A(p_{n}(2e_{1}))) + 0.\]
Subtracting these two equations, we get \[p_{n+1}(e_1) - p_{n+1}(2e_1) \ge p_{n}(e_{1})- p_{n}(2e_{1}) + {2d+1 \over 2d} (A(p_{n}(2e_{1})) - A(p_{n}(e_{1}))).\] Now, arguing as in the proof of Lemma 9, by the mean-value theorem, \[\begin{gather} (p_{n}(e_{1})- p_{n}(2e_{1}))\left[1 - {2d + 1 \over 2d} \left({A(p_{n}(2e_{1})) - A(p_{n}(e_{1})) \over (p_{n}(e_{1})- p_{n}(2e_{1}))}\right)\right]\\ = (p_{n}(e_{1})- p_{n}(2e_{1}))\left[1 - {2d+1 \over 2d} A'(t)\right], \end{gather}\] for some \(t \in [p_{n}(2e_{1}), p_{n}(e_{1})]\). Since \(A'(t) \le 2/3\) whenever \(0 \le t \le 1/3\) and \((2d+1)/2d \le 3/2\), the above expression is at least \((p_{n}(e_{1})- p_{n}(2e_{1})) [1 - (3/2) (2/3)] = 0\).
Case 2. \(k= e_1 + e_2\).
We perform a similar analysis as above. We have that for \(\ell\sim e_{1}+e_{2}\), by symmetry, \[p_{n}(\ell)\begin{cases} \leq p_n(2e_{1})&\text{if \ell=2e_1+e_{2}, e_{1}+2e_{2}},\\ =p_{n}(e_{1})&\text{if \ell=e_{1}, e_{2}},\\ \leq p_{n}(e_{1}+e_{2})&\text{otherwise}. \end{cases}\] This implies \[p_{n+1}(e_1 + e_2) \le p_{n}(e_{1}+e_{2}) + {2 \over 2d} (A(p_n(e_1)) - A(p_{n}(e_{1}+e_{2}))) + {2 \over 2d} (A(p_n(2e_1)) - A(p_{n}(e_{1}+e_{2}))).\] Subtracting this from the inequality for \(p_{n+1}(e_1)\) from the first case, we obtain the bound \[p_{n+1}(e_1) - p_{n+1}(e_1 + e_2) \ge p_{n}(e_{1}) - p_{n}(e_{1}+e_{2}) + {2d+2 \over 2d} (A( p_{n}(e_{1}+e_{2})) - A(p_{n}(e_{1}))).\] Since again, \(A'(t) \le 2/3\) whenever \(0\leq t \le 1/3\), and \((2d+2)/2d \le 3/2\) because \(d \ge 2\), this implies the right side is at least 0.
Finally, we must also show that \(p_{n+1}(k) \le p_{n+1}(0)\) if \(|k|_1 \ge 2\). In this case, because \(p_n\) is almost-volcanic, \(p_n(k) \le p_n(0)\) and all the neighbours \(\ell\sim k\) have \(p_n(\ell) \le p_n(e_1)\), so since \(A\) is increasing, \[\begin{align} p_{n+1}(k) &= p_n(k) + {1 \over 2d} \sum_{\ell\sim k} (A(p_n(\ell)) - A(p_n(k))) \\&\le p_n(k) + {1 \over 2d} \sum_{\ell\sim k} (A(p_n(e_1)) - A(p_n(k))). \end{align}\] If we remove all \(A(p_n(k))\) terms out of the sum, and using that \(t\mapsto t-A(t)\) is nondecreasing for \(0\leq t\leq 1/3\), we get \[\begin{align} p_{n+1}(k) &\le p_n(k) - A(p_n(k)) + {1 \over 2d} \sum_{\ell\sim k} A(p_n(e_1)) \\&\le p_n(0) - A(p_n(0)) + {1 \over 2d} \sum_{\ell\sim k} A(p_n(e_1)) \\&=p_{n+1}(0). \end{align}\] This proves the second condition, so \(p_{n+1}\) is indeed almost-volcanic. ◻
Since \(d \ge 2\), \[p_1(k)=\begin{cases}1/2d&\text{when k\sim 0},\\ 0&\text{otherwise,} \end{cases}\] which is clearly almost-volcanic, so by the prior result, \(p_n\) is also almost-volcanic for any \(n \ge 1\). In the rest of this section we suppose that \(p_n\) is almost-volcanic for all \(n\geq 1\). We can use this with the bound in Theorem 2(i) to get a bound on the total variation of \(p_n\), for all \(n\geq 1\).
Proof of Theorem 2(iii). In order to estimate \([p_{n}]_{\mathop{\mathrm{TV}}(D)} := \tfrac{1}{2}\sum_{\{u,v\in D: u\sim v\}} |p_{n}(v)-p_{n}(u)|\) on the set \(D := B(rn^\beta) \cap \mathbb{Z}^d\), we observe that since both the set \(D\) and the almost-volcanic function \(p_{n}\) are invariant under reflection and coordinate transposition, we may reduce this expression to studying \[[ p_n ]_{\mathop{\mathrm{TV}}(D)} = d \sum_{k\in \mathcal{D}}\;|p_n(k+ e_1) - p_n(k)|,\] where \[\mathcal{D}:=\left\{k\in \mathbb{Z}^d: k, k+e_1 \in D\right\}.\]
Let \[\overline{p}_{n}(k) = \begin{cases} p_n(e_{1})&\text{if k=0},\\ p_{n}(k)&\text{otherwise.} \end{cases}\] This makes \(\overline{p}_{n}\) a volcanic function, and this implies that \[\overline{p}_{n}(k+ e_1) - \overline{p}_{n}(k)=\begin{cases}\geq 0&\text{if k_{1}<0},\\ \leq 0&\text{if k_{1}\geq 0.} \end{cases}\] For each \(k\in \mathcal{D}\), we rewrite \(k=(k_{1}, k')\) where \(k'\in \mathbb{Z}^{d-1}\), and for such \(k'\), we denote that \(k'\in \mathcal{D}'\). We now estimate the total variation of \(\overline{p}_{n}\), which by the prior observation and symmetry is given by, \[\begin{align} d\sum_{k\in \mathcal{D}}& |\overline{p}_{n}(k+ e_1) - \overline{p}_{n}(k)| \\ &= d \sum_{k'\in \mathcal{D}'} \Bigg[\sum_{k_{1}<0: (k_{1}, k')\in \mathcal{D}} \overline{p}_{n}(k+ e_1) - \overline{p}_{n}(k)+\sum_{k_{1}\geq 0: (k_{1}, k')\in \mathcal{D}} \overline{p}_{n}(k) - \overline{p}_{n}(k+ e_1)\Bigg]\\ &=d \sum_{k'\in \mathcal{D}'} [\overline{p}_{n}(0, k')-\overline{p}_{n}(-B+1, k')+\overline{p}_{n}(0, k')-\overline{p}_{n}(B+1, k')]\\ &\leq 2d \sum_{k'\in \mathcal{D}'} \overline{p}_{n}(0, k'), \end{align}\] where the point \(B\) is such that \((B, k')\in \mathcal{D}\) and \((B+1, k')\notin \mathcal{D}\).
Since \(\mathcal{D}\) (and hence \(\mathcal{D}'\)) has radius at most \(rn^\beta\), in order for \(k'\in \mathcal{D}'\), we must have \(|k_i| \le rn^\beta\) for \(i = 2, \ldots, d\). Therefore the sum has at most \((2rn^\beta)^{d-1}\) terms. By Theorem 2(i), each term is at most \(c/n^{d\beta}\), and thus \[[ \overline{p}_n ]_{\mathop{\mathrm{TV}}(\mathcal{D})}\leq cr^{d-1}n^{-\beta}.\]
We now compare the total variation of \(p_n\) to the total variation of \(\overline{p}_{n}\). Since only the origin of \(p_{n}\) differs from the origin of \(\overline{p}_{n}\), we have \[[ p_n ]_{\mathop{\mathrm{TV}}(D)}\leq [ \overline{p}_n ]_{\mathop{\mathrm{TV}}(D)}+2d|p_n(e_1) - p_n(0)|.\] Again by Theorem 2(i), the second term is bounded above by \(cn^{-d\beta}\), and hence \[[ p_n ]_{\mathop{\mathrm{TV}}(D)}\leq cr^{d-1}n^{-\beta}+cn^{-d\beta}.\]
If \(r < n^{-\beta}\), then \(D=\left\{0\right\}\), and by definition \([p_{n}]_{\mathop{\mathrm{TV}}(D)}=0\). Otherwise \(cn^{-d\beta} = c(n^{-\beta})^{d-1}n^{-\beta} \le cr^{d-1}n^{-\beta}\) and the total variation of \(p_{n}\) is at most \(cr^{d-1}n^{-\beta}\), which implies the claimed bound. ◻
In this section, we complete the proof of our main result, Theorem 1, by situating the central limit theorem as a consequence of the convergence of a finite difference scheme. As priorly mentioned, to our knowledge, there is no general theory of convergence for finite difference schemes approximating the porous medium equation with initial data which do not belong to \(L^\infty(\mathbb{R}^{d})\). Theorem 2 is used crucially throughout our argument.
For an interval \(I \subset [0,\infty)\), we let \[\begin{gather} C(I;L^{1}(\mathbb{R}^{d})) = \{u: \mathbb{R}^{d} \times I \to \mathbb{R}\mid u(\cdot,t) \in L^{1}(\mathbb{R}^{d}) \text{ for all }t \in I, \text{ and} \\ \lim_{t \to t_{0}}\|u(\cdot,t)-u(\cdot,t_{0})\|_{L^{1}(\mathbb{R}^d)} = 0 \text{ for all }t_{0} \in I \}. \end{gather}\] We rely on continuity properties of functions with respect to the \(L^{1}(\mathbb{R}^{d})\) norm. We refer to a modulus of continuity as a function \(\nu:[0,\infty)\to [0,\infty)\) which is nondecreasing, continuous at \(0\), and for which \(\nu(0) = 0\). In the rest of this section, we assume that \(\nu\) is a modulus of continuity. We say that a function \(w \in L^{1}(\mathbb{R}^{d})\) has spatial modulus of continuity \(\nu\) if \[\|w(\cdot + y) - w(\cdot)\|_{L^{1}(\mathbb{R}^{d})} \leq \nu(|y|)\quad\text{for all y\in \mathbb{R}^{d}}.\] For an interval \(I\subset [0,\infty)\), we say that \(v \in L^{1}(\mathbb{R}^{d} \times I)\) has spatial modulus of continuity \(\nu\) if \[\|v(\cdot+y,t)-v(\cdot,t)\|_{L^1(\mathbb{R}^d)} \le \nu(|y|)\quad\text{for all t\in I and y\in \mathbb{R}^{d}}\, ,\] and that \(v\) has temporal modulus of continuity \(\nu\) if, \[\|v(\cdot,t) - v(\cdot,s)\|_{L^{1}(\mathbb{R}^{d})} \leq \nu(|t-s|)\quad\text{for all s,t \in I.}\] We say a collection \((v_a)_{a \in A}\subset L^1(\mathbb{R}^d\times I)\) has spatial (resp.temporal) modulus of continuity \(\nu\) if for every \(a\in A\), \(v_a\) has spatial (resp.temporal) modulus of continuity \(\nu\). Note that if \(v \in L^{1}(\mathbb{R}^{d} \times I)\) has a temporal modulus of continuity on \(\mathbb{R}^{d} \times I\), then \(v \in C(I;L^{1}(\mathbb{R}^{d}))\). Conversely, if \(I\) is a bounded interval and \(v \in C(I; L^{1}(\mathbb{R}^{d}))\) then \(v\) has a temporal modulus of continuity on \(\mathbb{R}^{d}\times I\). Lastly, for an arbitrary interval \(I \subset [0,\infty)\), we say that a sequence of functions \((v_{N})_{N\in{\mathbb{N}}}\) defined on \(\mathbb{R}^{d} \times I\) has approximate temporal modulus of continuity \(\nu\) on \(\mathbb{R}^{d}\times I\) if for all \(N \in {\mathbb{N}}\) and all \(s,t\in I\), \[\|v_{N}(\cdot,t) - v_{N}(\cdot,s)\|_{L^{1}(\mathbb{R}^{d})} \leq \nu(|s-t|+\tfrac{1}{N}).\]
Remark 33. We remark that a modulus of continuity (be it spatial, temporal, or approximate temporal) is not unique; a modulus of continuity can always be replaced by any other modulus of continuity which dominates it. Hence, we will often assume without loss of generality that any two a priori distinct moduli of continuity are in fact the same.
We define two notions of solution for the Cauchy problem \[\label{e46pme} \begin{cases} u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0 &\text{in } Q_{T}=\mathbb{R}^{d}\times (0,T], \\ u(x,0) = u_{0}(x) &\text{in \mathbb{R}^{d}}. \end{cases}\tag{58}\] Our work builds upon that of Karlsen and Risebro [10]. In that article, they work with a nonnegative entropy solution, which is defined as follows.
Definition 1. For \(T > 0\), we say that a measurable function \(u: Q_{T}\to \mathbb{R}\) is a nonnegative entropy solution to the equation \(u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0\) in \(Q_{T}\) if the following holds:
\(u \in L^{1}(Q_{T}) \cap L^{\infty}(Q_{T}) \cap C((0,T);L^{1}(\mathbb{R}^{d}))\).
\(u \geq 0\) a.e. in \(Q_{T}\).
For all \(c \in \mathbb{R}\) and all non-negative \(\varphi\in C^{\infty}_{c}(\mathbb{R}^{d} \times [0,T])\), \[\label{e46etrpycond} \int_{\mathbb{R}^{d}}\int_{0}^{T}\left(|u-c|\varphi_{t} +\left|u^{m+1}-c^{m+1}\right|\frac{1}{2d}\Delta \varphi\right)\,dt\,dx \geq 0.\tag{59}\]
\(u^{m+1} \in L^{2}((0,T) ;H^{1}(\mathbb{R}^{d})),\) where \(H^{1}(\mathbb{R}^{d})\) is the Sobolev space \(W^{1,2}(\mathbb{R}^{d})\).
Definition 2. Let \(u_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\). For \(T > 0\), we say \(u: Q_{T}\to \mathbb{R}\) is a nonnegative entropy solution to 58 (the initial value problem) if it is a nonnegative entropy solution in the above sense and as \(t \to 0^{+}\), \(\|u(\cdot,t) - u_{0}\|_{L^{1}(\mathbb{R}^{d})} \to 0.\)
Remark 34. We remark that the definition in [10] is for a more general PDE, and we tailor the definition presented here to reflect the special case we are interested in. Furthermore, we require that \(u \geq 0\) a.e. in order to ensure that \(u \mapsto u^{m+1}\) is a nondecreasing function. In Remark 49, we further outline the details of how our setting is a specific case of the one considered in [10].
Remark 35. If \(u\in L^{1}(Q_{T}) \cap L^{\infty}(Q_{T}) \cap C((0,T);L^{1}(\mathbb{R}^{d}))\) is a nonnegative entropy solution to the initial value problem 58 , we can take the convention of defining \(u(x,0) := u_{0}(x)\). Hence, the convergence \(\|u(\cdot,t)-u_{0}\|_{L^{1}(\mathbb{R}^{d})} \to 0\) allows us to conclude that in fact \(u \in C([0,T); L^{1}(\mathbb{R}^{d}))\) instead of merely \(u \in C((0,T);L^{1}(\mathbb{R}^{d}))\).
There is another kind of solution to 58 which allows for distributional initial conditions, i.e. the case where \(u_{0}\) is a Radon measure.
Definition 3. For \(T > 0\), we say that a measurable function \(u: Q_{T}\to \mathbb{R}\) is a distributional solution of \(u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0\) in \(Q_{T}\) if
\(u \in L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})\), the space of locally integrable functions on \(Q_{T}\).
\(u^{m+1} \in L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})\).
\(u \in C((0,T);L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}))\).
For all \(\varphi\in C^{\infty}_{c}(Q_{T})\), we have \[\label{e46distIBP} \int_{\mathbb{R}^{d}} \int_{0}^{T} \left(u \varphi_{t} + (u^{m+1})\frac{1}{2d}\Delta\varphi\right)\,dt\,dx = 0.\tag{60}\]
We remark that in the above definition, condition (3) is immediate from the other conditions by the following theorem.
Theorem 36 ([6], Theorem 13.16). For \(T > 0\), let \(u: Q_{T}\to \mathbb{R}\) be a measurable function satisfying conditions (1), (2), and (4) of Definition 3. Then, \(u\) is locally Hölder continuous, in particular \(u \in C(Q_{T})\) and \(u \in C((0,T); L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}))\).
As for the initial conditions of a distributional solution, we have the following definition.
Definition 4. Let \(u_{0}\) be a Radon measure on \(\mathbb{R}^{d}\). We say that \(u\) is a distributional solution of 58 (the initial value problem) if \(u\) is a distributional solution in the above sense, and if for all \(\varphi\in C_{c}(\mathbb{R}^{d})\), \[\lim_{t \to 0^{+}} \int_{\mathbb{R}^{d}}u(x,t)\varphi(x) \,dx = \int_{\mathbb{R}^{d}} \varphi(x) u_{0}(dx).\] In such a case we call \(u_{0}\) the initial trace of \(u\). For \(u_{0} \in L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\), we use the embedding of \(u_{0}\) as a Radon measure, namely \(u_{0}(dx) = u_{0}\,dx\), in the above definition.
We remark that if \(u_{0} \in L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\), the above definition is equivalent to saying \(u(\cdot,t) \xrightarrow{t\to 0^{+} }u_{0}\), in \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\), and is thus consistent with the way we interpret initial conditions for nonnegative entropy solutions, albeit for convergence in \(L^1_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\) instead of \(L^1(\mathbb{R}^{d})\).
The reason for introducing distributional solutions is that they allow for a theory of uniqueness, even when the initial condition \(u_{0}\) is a Radon measure.
Theorem 37 ([6], Theorem 13.8). For \(T > 0\), let \(u_{1}\) and \(u_{2}\) be two nonnegative distributional solutions of \(u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0\) in \(Q_{T}\). If the initial traces of both \(u_{1}\) and \(u_{2}\) coincide, then \(u_{1} = u_{2}\) a.e. in \(Q_{T}\).
Remark 38. In [6], the result is for uniqueness of continuous nonnegative distributional solutions. However, by Theorem 36, all distributional solutions have an a.e. continuous representative. Hence we can state Theorem 37 in the form given.
Lastly, we show that all nonnegative entropy solutions are in fact distributional solutions.
Proposition 39. Let \(u\) be a nonnegative entropy solution to \(u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0\) in \(Q_{T}\). Then \(u\) is a distributional solution to \(u_{t} - \frac{1}{2d}\Delta(u^{m+1}) = 0\) in \(Q_{T}\).
Proof. We remark that \(u \in L^{\infty}(Q_{T})\) implies that \(u, u^{m+1} \in L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})\). Therefore all that remains to be shown is the integration by parts formula 60 . Let \(\varphi\in C^{\infty}_{c}(Q_{T})\). First, we assume \(\varphi\geq 0\). By choosing \(c = 0\) in 59 , we have \[\int_{\mathbb{R}^{d}}\int_{0}^{T}\left(u\varphi_{t} +u^{m+1}\frac{1}{2d}\Delta \varphi\right)\,dt\,dx \geq 0.\] Next, by choosing \(c = \|u\|_{L^{\infty}(Q_{T})}\) in 59 , we have \[\int_{\mathbb{R}^{d}}\int_{0}^{T}\left((\|u\|_{L^{\infty}(Q_{T})}-u)\varphi_{t} +\left(\|u\|_{L^{\infty}(Q_{T})}^{m+1}-u^{m+1}\right)\frac{1}{2d}\Delta \varphi\right)\,dt\,dx \geq 0,\] which implies \[\begin{align} \int_{\mathbb{R}^{d}}\int_{0}^{T}\left(u\varphi_{t} +u^{m+1}\frac{1}{2d}\Delta \varphi\right)\,dt\,dx &\leq \int_{\mathbb{R}^{d}}\int_{0}^{T}\left(\|u\|_{L^{\infty}(Q_{T})}\varphi_{t} +\|u\|_{L^{\infty}(Q_{T})}^{m+1}\frac{1}{2d}\Delta \varphi\right)\,dt\,dx\\ & = 0, \end{align}\] where we used the fundamental theorem of calculus and the compact support of \(\varphi\) in the last step. Hence, we conclude that 60 holds for for all \(\varphi\in C^{\infty}_{c}(Q_{T})\) with \(\varphi\geq 0\). To account for general \(\varphi\in C^{\infty}_{c}(Q_{T})\), we decompose \(\varphi\) into \(\varphi= \varphi^{+} - \varphi^{-}\) for \(\varphi^{+}, \varphi^{-} \geq 0\) and \(\varphi^{+}\varphi^{-} \equiv 0\). We note that \(\varphi^{+}\) and \(\varphi^{-}\) may not be smooth at their \(0\)-level sets. However, by approximating each of \(\varphi^{+}\) and \(\varphi^{-}\) by smooth functions, we can still conclude 60 holds for both \(\varphi\) replaced by \(\varphi^{+}\) and for \(\varphi\) replaced by \(\varphi^{-}\). Finally, recalling \(\varphi= \varphi^{+} - \varphi^{-}\), we obtain the desired result for \(\varphi\). ◻
By combining Theorems 37 and Proposition 39 we obtain the following result.
Corollary 40. Let \(T > 0\) and \(u_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\). If \(u_{1}\) and \(u_{2}\) are two nonnegative entropy solutions to 58 , then \(u_{1} \overset{a.e.}{=} u_{2}\).
Remark 41. We remark that by considering the function \(\tilde{u}(x,t) := u(x,t+a)\), one can adapt the two definitions of solutions presented above to domains of the form \(\mathbb{R}^{d}\times (a,b)\).
In this section, we outline some of the tools and technical lemmas that we will use throughout the rest of this section.
We begin with a compactness result for \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times[a,b])\).
Lemma 42 ([18], Lemma 3.3). Let \((v_{N})_{N \in {\mathbb{N}}}\) be a sequence of functions defined on \(\mathbb{R}^{d} \times [a,b]\) which satisfies the following conditions:
There exists \(C> 0\) such that for all \(N \in {\mathbb{N}}\) and \(t \in [a,b]\), \[\|v_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} \leq C \text{ and } \|v_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})} \leq C.\]
There exists a spatial modulus of continuity \(\nu\) such that for all \(N\in {\mathbb{N}}\) and \(t \in [a,b]\), \[\|v_{N}(\cdot + y,t) - v_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} \leq \nu(|y|).\]
There exists an approximate temporal modulus of continuity \(\omega\) such that for all \(N \in {\mathbb{N}}\) and \(s, t \in [a,b]\), \[\|v_{N}(\cdot,t) - v_{N}(\cdot,s)\|_{L^{1}(\mathbb{R}^{d})} \leq \omega(|t-s| + \tfrac{1}{N}).\]
Then \((v_{N})_{N\in {\mathbb{N}}}\) is compact in the strong topology of \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times[a,b])\). Moreover, if \(v\) is an \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times[a,b])\)-limit point of \((v_{N})_{N \in {\mathbb{N}}}\), then \(v \in L^{1}(\mathbb{R}^{d}\times[a,b])\cap L^{\infty}(\mathbb{R}^{d}\times[a,b]) \cap C([a,b];L^{1}(\mathbb{R}^{d}))\), and \(v\) has a spatial modulus of continuity \(\nu\) on \(\mathbb{R}^{d}\times[a,b]\) and \(v\) has a temporal modulus of continuity \(\omega\) on \(\mathbb{R}^{d}\times[a,b]\).
Remark 43. We note that the reference [18] only concludes that \(v \in C((a,b);L^{1}(\mathbb{R}^{d}))\) and not that \(v \in C([a,b];L^{1}(\mathbb{R}^{d}))\). Because \(v\) admits \(\omega\) as a temporal modulus of continuity, \(t \mapsto v(\cdot,t)\) is uniformly continuous as a function from \([a,b]\) to \(L^{1}(\mathbb{R}^{d})\). Hence, because \(L^{1}(\mathbb{R}^{d})\) is complete, we can extend this mapping uniquely to define \(v(\cdot,a)\) and \(v(\cdot,b)\) as functions in \(L^{1}(\mathbb{R}^{d})\), and then \(v \in C([a,b];L^{1}(\mathbb{R}^{d}))\). The temporal continuity also implies that \(\nu\) is a spatial modulus of continuity on all of \(\mathbb{R}^{d}\times [a,b]\), and not merely \(\mathbb{R}^{d} \times (a,b)\).
Next, we state a technical lemma on the convergence of sequences of functions which admit a temporal modulus of continuity.
Lemma 44. Let \((w_{N})_{N \in {\mathbb{N}}}\) and \((z_{N})_{N \in {\mathbb{N}}}\) be two sequences in \(L^{1}(\mathbb{R}^{d}\times[a,b])\) which have an approximate temporal modulus of continuity \(\omega\). Then for all compact \(D \subset \mathbb{R}^{d}\), \[\|w_{N} - z_{N}\|_{L^{1}(D\times (a,b))} \xrightarrow{} 0 \text{ if and only if, for all } t \in [a,b], \|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \xrightarrow{} 0.\]
Proof. First, assume that \[\label{e46sliceloc} \|w_{N} - z_{N}\|_{L^{1}(D\times (a,b))} \xrightarrow{N \to \infty} 0.\tag{61}\] Fix \(t \in [a,b)\) and \(\varepsilon\in (0,b-t)\). We calculate \[\begin{align} &\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \\ &= \frac{1}{\varepsilon}\int_{t}^{t+\varepsilon}\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)}\,ds \\ &\leq \frac{1}{\varepsilon}\int_{t}^{t+\varepsilon}\|w_{N}(\cdot,t) - w_{N}(\cdot,s)\|_{L^{1}(D)}\,ds + \frac{1}{\varepsilon}\|w_{N} - z_{N}\|_{L^{1}(D\times(t,t+\varepsilon))} \\ &\quad\quad\quad\quad\quad\quad\quad+\frac{1}{\varepsilon}\int_{t}^{t+\varepsilon}\|z_{N}(\cdot,s) - z_{N}(\cdot,t)\|_{L^{1}(D)}\,ds. \end{align}\] We bound the final term in the upper bound by observing that \[\frac{1}{\varepsilon}\int_{t}^{t+\varepsilon}\|z_{N}(\cdot,s) - z_{N}(\cdot,t)\|_{L^{1}(D)}\,ds \leq \frac{1}{\varepsilon}\int_{t}^{t+\varepsilon}\omega(s-t+\tfrac{1}{N})\,ds \leq \omega(\varepsilon+\tfrac{1}{N}).\] A similar calculation holds for the first term in the upper bound, so we have \[\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \leq 2 \omega(\varepsilon+\tfrac{1}{N}) + \frac{1}{\varepsilon}\|w_{N} - z_{N}\|_{L^{1}(D\times(t,t+\varepsilon))}.\] Taking \(N \to \infty\) in the above, we apply 61 to obtain that for every \(t\in [a,b)\), \[\limsup_{N \to \infty}\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \leq 2 \omega(\varepsilon).\] Lastly, sending \(\varepsilon\to 0\) allows us to conclude that \(\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \to 0\). In the case \(t = b\), we can repeat a similar argument by instead integrating from \(t - \varepsilon\) to \(t\).
For the other implication, fix \(n \in {\mathbb{N}}\) and a partition \(\{t_{i}\}_{i = 0}^{n}\) of \([a,b]\) with \(t_{0} = a\) and \(t_{i}-t_{i-1} = \frac{b-a}{n}\). We then have \[\begin{align} &\|w_{N} - z_{N}\|_{L^{1}(D\times (t_{i-1},t_{i}))} \\ &\leq \int_{t_{i-1}}^{t_{i}}\|w_{N}(\cdot,s) - w_{N}(\cdot,t_{i})\|_{L^{1}(D)}\,ds + \int_{t_{i-1}}^{t_{i}}\|w_{N}(\cdot,t_{i})-z_{N}(\cdot,t_{i})\|_{L^{1}(D)}\,ds \\ & \quad\quad\quad\quad\quad\quad\quad+\int_{t_{i-1}}^{t_{i}}\|z_{N}(\cdot,t_{i}) - z_{N}(\cdot,s)\|_{L^{1}(D)}\,ds \\ &\leq 2\left(\tfrac{b-a}{n}\right)\cdot\omega\left(\tfrac{b-a}{n} + \tfrac{1}{N}\right) + \tfrac{b-a}{n}\|w_{N}(\cdot,t_{i})-z_{N}(\cdot,t_{i})\|_{L^{1}(D)} . \end{align}\] Therefore, \[\begin{align} \|w_{N} - z_{N}\|_{L^{1}(D\times (a,b))} &= \sum_{i = 1}^{n} \|w_{N} - z_{N}\|_{L^{1}(D\times (t_{i-1},t_{i}))} \\ &\leq 2\left(b-a\right)\cdot\omega\left(\tfrac{b-a}{n}+\tfrac{1}{N}\right) + \tfrac{b-a}{n}\sum_{i=1}^{n}\|w_{N}(\cdot,t_{i})-z_{N}(\cdot,t_{i})\|_{L^{1}(D)} \end{align}\] If for all \(t \in [a,b]\), \(\|w_{N}(\cdot,t) - z_{N}(\cdot,t)\|_{L^{1}(D)} \xrightarrow{N \to \infty} 0\), then it follows from the above that \[\limsup_{N \to \infty}\|w_{N} - z_{N}\|_{L^{1}(D\times (a,b))} \leq 2\left(b-a\right)\cdot\omega\left(\tfrac{b-a}{n}\right),\] and so we conclude by taking \(n \to \infty\). ◻
Our lemma yields the following corollary.
Corollary 45. For an interval \(I \subset \mathbb{R}\), let \(w,z \in L^{1}(\mathbb{R}^{d} \times I) \cap C(I;L^{1}(\mathbb{R}^{d}))\). Then \[w \overset{a.e.}{=} z \text{ in }\mathbb{R}^{d} \times I \text{ if and only if } w(\cdot,t) \overset{a.e.}{=} z(\cdot,t) \text{ in } \mathbb{R}^{d} \text{ for all } t \in I.\]
Proof. It suffices to prove the corollary assuming \(I\) is compact; so write \(I=[a,b]\) for \(a,b \in \mathbb{R}\). Fix a compact \(D \subset \mathbb{R}^{d}\). Because \(w, z \in C([a,b];L^{1}(\mathbb{R}^{d}))\), both \(w\) and \(z\) have temporal moduli of continuity on \(\mathbb{R}^{d}\times[a,b]\). By Remark 33, without loss of generality, we can assume these moduli to be the same. Thus, we apply Lemma 44 to the constant sequences \(w_{N} \equiv w\) and \(z_{N} \equiv z\) to obtain \[\|w - z\|_{L^{1}(D \times [a,b])} = 0 \text{ if and only if } \|w(\cdot,t)-z(\cdot,t)\|_{L^{1}(D)}=0 \text{ for all } t \in [a,b].\] Because \(D\) and \([a,b]\) are arbitrary, the result follows. ◻
Finally, we state a result which, under certain hypotheses, allows us to upgrade a spatial modulus of continuity to a temporal modulus of continuity.
Lemma 46 (Kružkov’s interpolation lemma [19]). Let \(z \in L^{\infty}(\mathbb{R}^{d}\times[0,T])\). Assume that \(z\) has a spatial modulus of continuity \(\nu\) on \(\mathbb{R}^{d}\times[0,T]\). Given \(C>1\), if \(t_1, t_2 \in [0,T]\) are such that for all \(\varphi\in C^{\infty}_{c}(\mathbb{R}^{d})\), \[\label{e46KILhyp} \left| \int_{\mathbb{R}^{d}} (z(x,t_2)-z(x,t_{1})) \varphi(x) \, dx\right| \leq C\cdot\left(\sum_{i = 1}^{d} \|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}\right)\cdot |t_{2}-t_{1}|,\qquad{(2)}\] then for all \(\varepsilon> 0\), \[\|z(\cdot,t_{2}) - z(\cdot,t_{1})\|_{L^{1}(\mathbb{R}^{d})} \leq 2C \cdot \left( \frac{|t_{2}-t_{1}|}{\varepsilon^2} + \nu(\varepsilon)\right).\]
It is worth noting that hypothesis ?? is a simplified version of the more general result stated in [19].
We consider the case of diffuse initial conditions, meaning we consider the PDE \[\label{e46pmev} \begin{cases} v_{t} - \frac{1}{2d}\Delta(v^{m+1}) = 0 &\text{in }Q_{T} \\ v(x,0) = v_{0}(x) &\text{for }x \in \mathbb{R}^{d}, \end{cases}\tag{62}\] where \(v_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\). In this case, the discrete approximations \(v_{N}\) satisfy some useful properties, as outlined in the following lemma. To understand the lemma statement, recall the definition of \(\mathcal{S}_N\) from 15 with the choice of \(A(u)=u^{m+1}\), given by \[\mathcal{S}_{N}v(k\Delta_x)= v(k\Delta_x)+\frac{\Delta_t}{2d (\Delta_x)^2}\sum_{\ell \sim k}\left[(v(\ell \Delta_x))^{m+1}-(v(k\Delta_x))^{m+1}\right],\] and \(1/N=\Delta_t=\Delta_x^{1/\beta}\). We recall that for \(v_{0}\in L^{1}(\mathbb{R}^{d})\), we say that \(v_{N}\) is generated by \(\mathcal{S}_{N}\) with initial condition \(v_{0}\) has initial condition defined by 18 .
Lemma 47. Let \(v_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\) where \(v_{0} \geq 0\), and \(v_{0}\) has a spatial modulus of continuity \(\nu\). Let \(v_{N}\) be generated by \(\mathcal{S}_{N}\) with initial condition \(v_{0}\). Then, there exists \(N_{0} = N_{0}(d,m,\|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}) \in {\mathbb{N}}\) such that the following hold.
(i) For all \(N \geq N_{0}\), and \(t \geq 0\), \[\|v_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})} \leq \|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}\quad\text{and}\quad\|v_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} \leq \|v_{0}\|_{L^{1}(\mathbb{R}^{d})}.\]
(ii) For all \(N \in {\mathbb{N}}\), \(v_{N}\) admits \(\nu\) as a spatial modulus of continuity on \(\mathbb{R}^{d}\times[0,T]\).
(iii) The tail sequence \((v_{N})_{N \geq N_{0}}\) admits an approximate temporal modulus of continuity on \(\mathbb{R}^{d}\times[0,T]\).
Proof. To prove (i), fix \(t>0\), let \(n = \left\lfloor t/\Delta_t\right\rfloor\), \(\Lambda:= \|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}\), and define \[N_{0} := (4(m+1)\Lambda^{m})^{\frac{1}{dm\beta}}.\] For \(N \geq N_{0}\), \(N\) satisfies ?? , and so Lemma 8(i, ii) gives that \[0 \leq v_{N}(\cdot, t) = \mathcal{S}^{n}_{N}v_{0} \leq \bigg\|\frac{1}{\square_{N}}\int_{\square_{N}(\cdot)} v_{0}(x)\, dx\bigg\|_{L^{\infty}(\mathbb{Z}^{d}\Delta_x)}\leq \Lambda= \|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}.\] Furthermore, choosing \(w_{N} := v_{N}(\cdot,0)\) and \(w'_{N} \equiv 0\) in Lemma 8(iii) gives that \[\|v_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} = \|\mathcal{S}^n_{N}(v_{N}(\cdot,0))\|_{L^{1}(\mathbb{R}^{d})} \leq \|v_{N}(\cdot,0)\|_{L^{1}(\mathbb{R}^{d})} = \|v_{0}\|_{L^{1}(\mathbb{R}^{d})},\] and so (i) is proved.
To prove (ii), let \(N \in {\mathbb{N}}\). We remark that directly by definition 15 , \(\mathcal{S}_{N}\) is translation invariant, meaning that for \(y \in \mathbb{R}^{d}\), \[\big[\mathcal{S}_{N}v_{N}(\cdot + y)\big](x) = \big[\mathcal{S}_{N}v_{N}\big](x+y).\] We use the translation invariance of \(\mathcal{S}_{N}\), along with Lemma 8(iii), to obtain that for all \(t \geq 0\), \(y \in \mathbb{R}^{d}\), \[\|v_{N}(\cdot + y, t) - v_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} \leq \|v_{0}(\cdot+ y) - v_{0}(\cdot)\|_{L^{1}(\mathbb{R}^{d})} \leq \nu(|y|).\]
To show (iii), we will use Kružkov’s interpolation lemma (Lemma 46). Let \(\varphi\in C_{c}^{\infty}(\mathbb{R}^{d})\), and fix \(n_{1}, n_{2} \in {\mathbb{N}}_{0}\). We will show that there is a constant \(C>1\) such that \[\left| \int_{\mathbb{R}^{d}} (v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \, dx\right| \leq C\cdot\left(\sum_{i = 1}^{d} \|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}\cdot\right) |n_{2}\Delta_t-n_{1}\Delta_t|.\] First, we use the fact that \(v_{N}(\cdot,t)\) is \(\mathbb{Z}^{d}\)-piecewise constant for all \(t \geq 0\) to calculate \[\begin{align} &\int_{\mathbb{R}^{d}} (v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \, dx \\ &= \sum_{k \in \mathbb{Z}^{d}} \int_{\square_{N}(k\Delta_x)}(v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \, dx \\ &= \sum_{k \in \mathbb{Z}^{d}} (v_{N}(k\Delta_x,n_{2}\Delta_t)-v_{N}(k\Delta_x,n_{1}\Delta_t)) \int_{\square_{N}(k\Delta_x)}\varphi(x) \, dx. \end{align}\] Define \(\overline{\varphi}_{N}: \mathbb{Z}^{d}\Delta_x\to \mathbb{R}\) by \(\overline{\varphi}_{N}(k\Delta_x) := \int_{\square_{N}(k\Delta_x)}\varphi(x)\,dx\). Introducing the shorthand \(V^{n}_{k} := v_{N}(k\Delta_x,n\Delta_t)\), we can rewrite the last display as \[\int_{\mathbb{R}^{d}} (v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \, dx = \sum_{k \in \mathbb{Z}^{d}} (V^{n_{2}}_{k}-V^{n_{1}}_{k})\overline{\varphi}_{N}(k\Delta_x).\] Assume without loss of generality that \(n_{2} \geq n_{1}\). By a telescoping sum, we can write \[\label{e46KIL1} \int_{\mathbb{R}^{d}} (v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \,dx = \sum_{n=n_{1}}^{n_{2}-1}\sum_{k \in \mathbb{Z}^{d}} (V^{n+1}_{k}-V^{n}_{k})\overline{\varphi}_{N}(k\Delta_x).\tag{63}\] For a fixed \(n \in {\mathbb{N}}_{0}\), we use the scheme satisfied by \(v_{N}\) to calculate \[\begin{align} \label{e46beforeFTC} &\sum_{k \in \mathbb{Z}^{d}} (V^{n+1}_{k}-V^{n}_{k})\overline{\varphi}_{N}(k\Delta_x) \notag\\ &= \frac{\Delta_t}{2d(\Delta_x)^{2}} \sum_{k \in \mathbb{Z}^{d}} \sum_{i=1}^{d} \left[(V^{n}_{k+e_{i}})^{m+1}-2(V^{n}_{k})^{m+1}+(V^{n}_{k-e_{i}})^{m+1}\right]\overline{\varphi}_{N}(k\Delta_x) \notag\\ &= \frac{\Delta_t}{2d(\Delta_x)^{2}} \sum_{k \in \mathbb{Z}^{d}} \sum_{i=1}^{d} (V^{n}_{k})^{m+1}\left[\overline{\varphi}_{N}((k+e_{i})\Delta_x) - 2\overline{\varphi}_{N}(k\Delta_x) + \overline{\varphi}_{N}((k-e_{i})\Delta_x)\right], \end{align}\tag{64}\] where in the last step we used summation by parts and the fact that \(\varphi\) has compact support. For a fixed \(i \in [d]\), we remark that \[\begin{align} &|\overline{\varphi}_{N}((k+e_{i})\Delta_x) - 2\overline{\varphi}_{N}(k\Delta_x) + \overline{\varphi}_{N}((k-e_{i})\Delta_x)| \\ & \leq \int_{\square_{N}(k\Delta_x)} \left|\left(\varphi(x+e_{i}\Delta_x)-\varphi(x)\right) - \left(\varphi(x) - \varphi(x-e_{i}\Delta_x)\right)\right|\,dx\\ &= \int_{\square_{N}(k\Delta_x)}\bigg| \int_{0}^{\Delta_x}\left[\partial_{x_{i}}\varphi(x + s_{1}e_{i}) - \partial_{x_{i}}\varphi(x + (s_{1}-\Delta_x)e_{i})\right]\,ds_{1}\bigg| dx \\ &= \int_{\square_{N}(k\Delta_x)}\bigg|\int_{0}^{\Delta_x}\int_{0}^{\Delta_x}\partial_{x_{i}}^{2}\varphi(x + (s_{1}+s_{2}-\Delta_x)e_{i})\,ds_{1}\,ds_{2}\bigg|\, dx. \end{align}\] Using now that \(|\square_{N}(k\Delta_x)|=(\Delta_x)^{d}\), we conclude that \[|\overline{\varphi}_{N}((k+e_{i})\Delta_x) - 2\overline{\varphi}_{N}(k\Delta_x) + \overline{\varphi}_{N}((k-e_{i})\Delta_x)| \leq \|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}(\Delta_x)^{d+2}.\] Returning to 64 , we deduce that \[\begin{align} \left|\sum_{k \in \mathbb{Z}^{d}} (V^{n+1}_{k}-V^{n}_{k})\overline{\varphi}_{N}(k\Delta_x)\right| &\leq \frac{\Delta_t}{2d(\Delta_x)^{2}} \sum_{k \in \mathbb{Z}^{d}} \sum_{i=1}^{d}(V^{n}_{k})^{m+1}\|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}(\Delta_x)^{d+2} \\ &= \frac{\Delta_t}{2d} \cdot\left((\Delta_x)^{d}\sum_{k \in \mathbb{Z}^{d}} (V^{n}_{k})^{m+1}\right) \cdot \left( \sum_{i=1}^{d}\|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}\right). \end{align}\] Because \(V^{n}_{k}:= v_{N}(k\Delta_x,n\Delta_t)\) and \(v_{N}(\cdot,n\Delta_t)\) is \(\mathbb{Z}^{d}\)-piecewise constant, \[\begin{align} (\Delta_x)^{d}\sum_{k \in \mathbb{Z}^{d}} (V^{n}_{k})^{m+1} &= \int_{\mathbb{R}^{d}}(v_{N}(x,n\Delta_t))^{m}v_{N}(x,n\Delta_t) \, dx \\ &\leq \|v_{N}(\cdot,n\Delta_t)\|_{L^{\infty}(\mathbb{R}^{d})}^{m} \|v_{N}(\cdot,n\Delta_t)\|_{L^{1}(\mathbb{R}^{d})}. \end{align}\] By property (i) since \(N\geq N_{0}\), we combine the previous two displays to obtain a constant \(C_{v_{0}}\), where \(C_{v_{0}} = C_{v_{0}}(d,m,\|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}, \|v_{0}\|_{L^{1}(\mathbb{R}^{d})}) > 0\), such that \[\left|\sum_{k \in \mathbb{Z}^{d}} (V^{n+1}_{k}-V^{n}_{k})\overline{\varphi}_{N}(k\Delta_x)\right| \leq C_{v_{0}} \Delta_t\left( \sum_{i=1}^{d}\|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}\right).\] Thus, returning to 63 , we have \[\begin{align} \left|\int_{\mathbb{R}^{d}} (v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)) \varphi(x) \,dx \right| &= \sum_{n=n_{1}}^{n_{2}-1} \left|\sum_{k \in \mathbb{Z}^{d}} (V^{n+1}_{k}-V^{n}_{k})\overline{\varphi}_{N}(k\Delta_x)\right| \\ &\leq C_{v_{0}}|n_{2}\Delta_t-n_{1}\Delta_t| \left( \sum_{i=1}^{d}\|\partial_{x_{i}}^{2}\varphi\|_{L^{\infty}(\mathbb{R}^{d})}\right). \end{align}\] Next, an application of Kružkov’s interpolation lemma (Lemma 46), with the choice \(\varepsilon= |n_{2}\Delta_t-n_{1}\Delta_t|^{1/3}\), yields, for all \(n_{1},n_{2} \in {\mathbb{N}}\), \[\begin{align} \int_{\mathbb{R}^{d}} |v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)| \varphi(x) \,dx&\leq 2C_{v_{0}}\big(|n_{2}\Delta_t-n_{1}\Delta_t|^{1/3} + \nu\big(|n_{2}\Delta_t-n_{1}\Delta_t|^{1/3}\big) \big) \\ &:= \omega(|n_{2}\Delta_t-n_{1}\Delta_t|), \end{align}\] where we remark that \(\omega= \omega(d,m,\|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}, \|v_{0}\|_{L^{1}(\mathbb{R}^{d})},\nu)\).
To conclude, we consider times which are not on the grid \({\mathbb{N}_{0}}\Delta_t\). Let \(t_{1},t_{2} \in [0,T]\). We have, by setting \(n_{1} = \left\lfloor t_{1}/\Delta_t\right\rfloor\) and \(n_{2} = \left\lfloor t_{2}/\Delta_t\right\rfloor\), that \[|n_{2}\Delta_t- n_{1}\Delta_t| \leq |t_{2}-t_{1}| + 2\Delta_t.\] Because \(v_{N}\) is piecewise constant in time, we conclude that, \[\begin{align} \int_{\mathbb{R}^{d}} |v_{N}(x,t_{2})-v_{N}(x,t_{1})| \,dx &= \int_{\mathbb{R}^{d}} |v_{N}(x,n_{2}\Delta_t)-v_{N}(x,n_{1}\Delta_t)| \,dx\\ &\leq \omega(|n_{2}\Delta_t-n_{1}\Delta_t|) \\ &\leq \omega(|t_{2}-t_{1}| + 2\Delta_t)\\ &\leq \omega(2(|t_{2}-t_{1}| +\tfrac{1}{N})), \end{align}\] where we used the fact that \(\Delta_t= N^{-1}\) in the final step. ◻
We now state a convergence result due to Karlsen and Risebro [10], which also yields an existence result for entropy solutions of the PME with “diffuse” initial conditions.
Theorem 48. [10] Let \(\Lambda> 0\), and \(A: [0,\Lambda] \to \mathbb{R}\) be a function such that \[\label{e46ahyp} A \text{ is non-decreasing, } A(0) = 0, \text{ and }A\text{ is Lipschitz continuous}.\qquad{(3)}\] Let \(v_{0} \in L^{1}(\mathbb{R}^{d}) \cap \mathcal{B}_{\Lambda}^{+}(\mathbb{R}^{d})\), and let \(v_{N}\) be generated by \(\mathcal{S}_{N}\) with initial condition \(v_{0}\). If there exists \(\varepsilon\in (0,1)\) such that for all \(N\) sufficiently large, \[\label{e46cfleps} 2N^{-\frac{dm}{dm+2}}\max_{r \in [0,\Lambda]}A'(r) < 1 - \varepsilon,\qquad{(4)}\] then there is a function \(v: \mathbb{R}^{d}\times [0, \infty)\rightarrow \mathbb{R}\) (independent of \(\varepsilon\)) such that for any \(T>0\), \(v_{N} \to v\) in \(L^{1}_{\text{loc}}(Q_{T})\), and \(v\) is the unique entropy solution to \[\begin{cases} v_{t}-\frac{1}{2d}\Delta(A(v))=0&\text{in \mathbb{R}^{d}\times (0, \infty)},\\ v(0,x)=v_{0}(x)&\text{in \mathbb{R}^{d}}. \end{cases}\]
Remark 49. Here we make a few remarks about how we adapted the statement of [10] to our situation. First, we note that the authors consider a more general PDE of the form \(u_{t} + \mathop{\mathrm{div}}f(u) = \frac{1}{2d}\Delta A(u)\). We state their result with the choice \(f \equiv 0\) for simplicity.
Second, they consider a slightly different set of assumptions on the function \(A\). In [10], \(A\) is defined in \(\mathbb{R}\) rather than \([0,\Lambda]\), \(A\) is locally Lipschitz rather than Lipschitz, and in the condition ?? , \(\max_{r \in [0,\Lambda]}A'(r)\) is replaced by \(\sup_{r \in \mathbb{R}}A'(r)\). Because we seek to use \(A(r) = r^{m+1}\), we restrict the domain of \(A\), \(\mathcal{D}(A)\), so that \(\mathcal{D}(A) := [0,\Lambda]\), to ensure that \(A\) is non-decreasing and that \(\max_{r \in \mathcal{D}(A)}A'(r) < \infty\). This domain restriction is made without loss of generality: the proof [10] only relies on an analysis of \(A(v_{N})\) and we know that \(v_{N}(\cdot, t)\in \mathcal{B}_{\Lambda}^{+}(\mathbb{R}^{d})\) whenever \(v_{0} \in \mathcal{B}_{\Lambda}^{+}(\mathbb{R}^{d})\cap L^1(\mathbb{R}^{d})\) (for \(N\) sufficiently large, by Lemma 47(ii)).
Lastly, as discussed in the remarks preceding the statement of [10], this theorem is an existence result for nonnegative entropy solutions with initial condition \(v_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\), so long as the function \(A\) satisfies ?? , which are conditions independent of \(\Lambda\).
The following corollary rephrases the above convergence result for our specific case, when \(A(u)=u^{m+1}\).
Corollary 50. Let \(v_{0} \in L^{1}(\mathbb{R}^{d}) \cap L^{\infty}(\mathbb{R}^{d})\) with \(v_{0} \geq 0\). Let \(v\) be the unique nonnegative entropy solution to 62 and let \(v_{N}\) be generated by \(\mathcal{S}_{N}\) with initial condition \(v_{0}\). Then \[v_{N} \xrightarrow{L^{1}_{\text{loc}}(Q_{T})} v \text{ and }v_{N}(\cdot,t) \xrightarrow{L^{1}_{\text{loc}}(\mathbb{R}^{d})} v(\cdot,t)\text{ for all }t \in [0,T].\]
Proof. Taking \(\Lambda= \|v_{0}\|_{\infty}\), there is an a.e. representative for \(v_{0}\) which satisfies \(v_{0}\in \mathcal{B}_{\Lambda}^{+}(\mathbb{R}^{d})\). Let \(A(u) := u^{m+1}\). Because \(\max_{u\in[0,\Lambda]}A'(u) = A'(\Lambda) = (m+1)\Lambda^{m}\), we see that the condition ?? is satisfied with \(\varepsilon= \frac{1}{2}\), so long as \[N^{\frac{dm}{dm+2}} \geq 4(m+1)\Lambda^{m},\] which is also a sufficient condition to guarantee monotonicity of \(\mathcal{S}_{N}\) (as seen in Lemma 8). Therefore, the hypotheses of Theorem 48 are satisfied and thus \(v_{N} \to v\) in \(L^{1}_{\text{loc}}(Q_{T})\).
Next, we show the final claim of \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\) convergence on time slices. By Lemma 47(iii), there is some \(N_{0} = N_{0}(m,d,\|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})}) \in {\mathbb{N}}\) so that \(\{v_{N}\}_{N \geq N_{0}}\) admits an approximate temporal modulus of continuity \(\omega\) on \(\mathbb{R}^{d}\times[0,T]\). Because \(v\) is an \(L^{1}_{\text{loc}}(Q_{T})\)-limit point of \(\{v_{N}\}_{N \geq N_{0}}\), Lemma 42 gives that \(\omega\) is also a temporal modulus of continuity for \(v\). Thus, we apply Lemma 44 to the sequence \(w_{N} := v_{N}\) and the constant sequence \(z_{N} := v\) to conclude that we also have the convergence \(v_{N}(\cdot,t) \xrightarrow{L^{1}_{\text{loc}}(\mathbb{R}^{d})} v(\cdot,t)\), for all \(t \in [0,T]\). ◻
Recall that \(1/N=\Delta_t=\Delta_x^{1/\beta}\). We begin this section by proving some important properties about \(u_{N}: \mathbb{R}^{d} \times [0,\infty)\rightarrow [0, \infty)\), the unique \((\mathbb{Z}^{d}\Delta_x\times{\mathbb{N}_{0}}\Delta_t)\)-piecewise constant function defined by \[u_{N}(k\Delta_x,n\Delta_t) := \frac{1}{|\square_{N}|} {\mathbf{P}}\left\{X^{n} = k\right\} = \frac{1}{(\Delta_x)^{d}}p(k,n).\] Recall that Remark 7 showed that \(u_{N}\) can equivalently be defined as the function \(u_{N}\) generated by \(\mathcal{S}_{N}[A]\) with \(A(u) = u^{m+1}\) and initial measure \(\delta\).
Proposition 51. For \(N \in {\mathbb{N}}\), let \(u_{N}\) be generated by \(\mathcal{S}_{N}[A]\) with \(A(u) = u^{m+1}\) with initial measure \(\delta\). There is a constant \(C=C(m,d)>0\) such that the following holds:
(i) \(\int_{\mathbb{R}^{d}}u_{N}(x,t)\,dx = 1\) for all \(t \in [0,\infty)\).
(ii) For all \(t \in (0,\infty)\) and \(N \geq 2/t\), \[0 \leq u_{N}(\cdot,t) \leq Ct^{-d\beta}.\]
(iii) For all \(t \in (0,\infty)\), \(N \geq 2/t\), and \(r > 2\sqrt{d}\Delta_x\), \[\int_{|x| > r} u_{N}(x,t) \,dx\leq C\exp\left(- rt^{-\beta}/C\right).\]
(iv) For all \(t \in (0,\infty)\), \(N \geq 2/t\), and \(r > 2\sqrt{d}\Delta_x\), \[[u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} \leq Ct^{-d\beta}r^{d-1}.\]
Proof.
(i) Let \(t \in [0,\infty)\). Because \(u_{N}(\cdot,t)\), is \(\mathbb{Z}^{d}\Delta_x\)-piecewise constant, \[\begin{align} \int_{\mathbb{R}^{d}}u_{N}(x,t)\,dx = (\Delta_x)^{d}\sum_{k \in \mathbb{Z}^{d}} u_{N}(k\Delta_x,t) = \sum_{k \in \mathbb{Z}^{d}} p(k, \left\lfloor t/\Delta_t\right\rfloor) = \sum_{k \in \mathbb{Z}^{d}}{\mathbf{P}}\left\{X^{\left\lfloor t/\Delta_t\right\rfloor} = k\right\} = 1. \end{align}\]
(ii) By Theorem 2[p46Linfty], there is a constant \(C = C(m,d) > 0\), such that \[0 \leq p(k,n) \leq Cn^{-d\beta} \text{ for all } k \in \mathbb{Z}^{d}, n \in {\mathbb{N}}.\] Fix \(t \in (0,\infty)\), \(x \in \mathbb{R}^{d}\), and integer \(N \geq 2/t\). Choose \(k \in \mathbb{Z}^{d}\) such that \(x \in \square_{N}(k\Delta_x)\) and let \(n = \left\lfloor t/\Delta_t\right\rfloor\). Since \(\Delta_x= (\Delta_t)^{\beta}\), we have \[0 \leq u_{N}(x,t) = (\Delta_t)^{-d\beta} p(k,n) \leq (\Delta_t)^{-d\beta} Cn^{-d\beta} = C (n\Delta_t)^{-d\beta}.\] We conclude using the fact that \(N \geq 2/t\), meaning \(\frac{1}{2} t \geq \Delta_t\), so \(n \Delta_t\geq t - \Delta_t\geq \frac{1}{2} t.\)
(iii) Since \(r > 2\sqrt{d}\Delta_x\), we have that \(r - \sqrt{d}\Delta_x> \frac{1}{2}r\), and thus, \[\int_{|x| >r} u_{N}(x,t)\,dx \leq (\Delta_x)^{d}\sum_{|k\Delta_x| > r - \sqrt{d}\Delta_x} u_{N}(k\Delta_x,t)\leq \sum_{|k\Delta_x| \geq \frac{1}{2} r}p(k,\left\lfloor t/\Delta_t\right\rfloor).\] Let \(n = \left\lfloor t/\Delta_t\right\rfloor\). Since \(\Delta_x= \Delta_t^{\beta}\), \[\sum_{|k\Delta_x| \geq \frac{1}{2} r}p(k,\left\lfloor t/\Delta_t\right\rfloor) = \sum_{|k| \geq \frac{1}{2} r\Delta_t^{-\beta}}p(k,n) = \sum_{|k| \geq \frac{1}{2} r(n\Delta_t)^{-\beta}n^{\beta}}p(k,n).\] Combining the previous two displays, we can apply Theorem 2[p46conc] to conclude that there is some constant \(C = C(m,d)>0\), such that: \[\int_{|x| >r} u_{N}(x,t)\,dx \leq \sum_{|k| \geq \frac{1}{2} r(n\Delta_t)^{-\beta}n^{\beta}}p(k,n) \leq C\exp(-r(n\Delta_t)^{-\beta}/C).\] We conclude by noting that \(\Delta_t^{-1}= N \geq 2/t\) means \(\frac{1}{2} t \geq \Delta_t\) and so \(n\Delta_t\geq t - \Delta_t\geq \frac{1}{2} t\).
(iv) By Theorem 2[p46BV], there is a constant \(C = C(m,d) > 0\) such that \[\label{e46pBValpha} [p(\cdot,n)]_{\mathop{\mathrm{TV}}(B_{\alpha}\cap\mathbb{Z}^{d})} \leq C\alpha^{d-1}n^{-d\beta} \text{ for all } \alpha > 0, n \in {\mathbb{N}}.\tag{65}\] Define the \(s\)-superlevel set of \(u_{N}\) as \(E^{s}:= \{x \in \mathbb{R}^{d} : u_{N}(x,t) > s\}\), and \(E^{s}_{r} := E^{s} \cap B_{r}\). Using one of the equivalent definitions for total variation, we have \[\label{e46TVdef2} [u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} = \int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s}_{r}) \, ds,\tag{66}\] where \(\mathcal{H}^{d-1}\) is the \((d-1)\)-dimensional Hausdorff measure (see for example [20]). Because \(u_{N}(\cdot,t)\) is \(\mathbb{Z}^{d}\Delta_x\)-piecewise constant, it follows that \[\partial E^{s}_{r} \subset \bigcup_{k \in \mathbb{Z}^{d}} \partial\square_{N}(k\Delta_x).\] For \(k \in \mathbb{Z}^{d}\), and \(\ell \sim k\), define \(\partial_{\ell}\square_{N}(k\Delta_x)\) to be the face of the \(d\)-hypercube \(\square_{N}(k\Delta_x)\) which has normal vector \(\ell-k\). We can re-write \[\bigcup_{k \in \mathbb{Z}^{d}} \partial\square_{N}(k\Delta_x) = \bigcup_{k \in \mathbb{Z}^{d}}\bigcup_{\ell \sim k} \partial_{\ell}\square_{N}(k\Delta_x).\] We remark that for every \(k \sim \ell\), \(\partial_{\ell}\square_{N}(k\Delta_x) = \partial_{k}\square_{N}(\ell\Delta_x)\). Hence, the right hand side union (up to a set of \(\mathcal{H}^{d-1}\) measure zero) exactly “double counts” each hypercube face. Therefore, we can re-write the integral 66 as \[[u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} = \frac{1}{2}\sum_{k \in \mathbb{Z}^{d}} \sum_{\ell \sim k}\int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s}_{r} \cap \partial_{\ell} \square_{N}(k\Delta_x)) \, ds.\] Since \(E^{s}_{r}:= E^{s} \cap B_{r} \subset B_{r}\), if \(|k\Delta_x| \geq 2r\) then \(|k\Delta_x|> r + 2\sqrt{d}\Delta_x\) and so for all \(\ell\sim k\) in this range, \(\partial E^{s}_{r} \cap \partial_{\ell} \square_{N}(k\Delta_x) = \emptyset.\) Thus, we can localize the sum over \(k\) in the above display as \[\begin{align} \label{e46TVupperbnd} [u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} &= \frac{1}{2}\sum_{|k| < 2r(\Delta_x)^{-1}} \sum_{\ell\sim k}\int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s}_{r} \cap \partial_{\ell} \square_{N}(k\Delta_x)) \, ds \notag\\ &\leq \frac{1}{2}\sum_{\substack{|k|,|\ell| < 4r(\Delta_x)^{-1} \\ \ell \sim k}} \int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s} \cap \partial_{\ell} \square_{N}(k\Delta_x)) \, ds, \end{align}\tag{67}\] where we emphasize that we replaced \(E^{s}_{r}\) by \(E^{s}\) in the last step.
Next, for a fixed $k \in \mathbb{Z}^{d}$ and $i \in [d]$, we
analyze the term
$\int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s} \cap \partial_{k+e_{i}} \square_{N}(k\Delta_x)) \, ds$.
Define
$$\begin{align} s_{\min} &:= \min\{u_{N}(k\Delta_x,t), u_{N}((k+e_{i})\Delta_x,t)\}\\ s_{\max} &:= \max\{u_{N}(k\Delta_x,t), u_{N}((k+e_{i})\Delta_x,t)\},
\end{align}$$ so $u_{N}(\cdot,t)$ has a jump discontinuity of size
$s_{\max}-s_{\min}$ across the face
$\partial_{k+e_{i}} \square_{N}(k\Delta_x)$. Because of this jump
discontinuity, we have
$$\partial E^{s} \cap \partial_{k+e_{i}} \square_{N}(k\Delta_x) = \begin{cases} \partial_{k+e_{i}} \square_{N}(k\Delta_x) &\text{ for } s \in (s_{\min},s_{\max}]\\ \emptyset &\text{ otherwise}. \end{cases}$$
Hence, we calculate that
$$\begin{align} \int_{-\infty}^{\infty} \mathcal{H}^{d-1}(\partial E^{s} \cap \partial_{k+e_{i}} \square_{N}(k\Delta_x))\,ds &= \int_{s_{\min}}^{s_{\max}} \mathcal{H}^{d-1}(\partial_{k+e_{i}} \square_{N}(k\Delta_x))\,ds \\ &= (s_{\max}-s_{\min})\mathcal{H}^{d-1}(\partial_{k+e_{i}} \square_{N}(k\Delta_x)) \\ &= |u_{N}((k+e_{i})\Delta_x,t) - u_{N}(k\Delta_x,t)| (\Delta_x)^{d-1} \\ &= (\Delta_x)^{-1} |p(k+e_{i},\left\lfloor t/\Delta_t\right\rfloor) - p(k,\left\lfloor t/\Delta_t\right\rfloor)|.
\end{align}$$ Letting $n = \left\lfloor t/\Delta_t\right\rfloor$,
we combine the above display with @eq:e46TVupperbnd , letting
$\ell=k\pm e_{i}$, to obtain that
$$[u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} \leq (\Delta_x)^{-1} [p(\cdot,n)]_{\mathop{\mathrm{TV}}(B_{4r(\Delta_x)^{-1}}\cap\mathbb{Z}^{d})}.$$
By applying @eq:e46pBValpha and $\Delta_x= (\Delta_t)^{\beta}$,
this implies that
$$[u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} \leq (\Delta_x)^{-1} C (r (\Delta_x)^{-1})^{d-1}n^{-d\beta} = C r^{d-1}(n\Delta_t)^{-d\beta}.$$
Finally, we conclude by again using that $n \Delta_t\ge t/2$.
◻
Lemma 52. Fix \(\eta \in (0,T)\). Let \(u_{N}\) be generated by \(\mathcal{S}_{N}\) with initial measure \(\delta\). Then \((u_{N})_{N\geq 2/\eta}\) admits a spatial modulus of continuity \(\nu_{\eta}\) on \(\mathbb{R}^{d}\times[\eta,T]\), and \((u_{N})_{N \geq 2/\eta}\) admits an approximate temporal modulus of continuity \(\omega_{\eta}\) on \(\mathbb{R}^{d} \times [\eta,T]\).
Proof. Let \(t \in [\eta,T]\). We first show that \(u_{N}(\cdot,t)\) admits a spatial modulus of continuity \(\nu_{\eta}\). Let \(|y| \leq 1\) and \(r \geq 4\). Then by partitioning \(\mathbb{R}^{d}\), \[\begin{gather} \label{e46uNsmod} \|u_{N}(\cdot + y,t) - u_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})} = \|u_{N}(\cdot+y,t)-u_{N}(\cdot,t)\|_{L^{1}(B_{\frac{r}{2}})} \\+ \|u_{N}(\cdot+y,t)-u_{N}(\cdot,t)\|_{L^{1}(B_{\frac{r}{2}}^{c})}. \end{gather}\tag{68}\] We begin by bounding the second term of 68 . Note that for \(x \in \mathbb{R}^{d}\) with \(|x| > r/2\), we have \(|x+y| \geq |x|-|y| > r/2 - 1 \geq r/4\). Because \(u_{N}\) is nonnegative, Proposition 51[uN46conc] gives that there is a \(C = C(m,d) > 0\) such that \[\label{e46uNsmod1} \int_{|x| > r/2}|u_{N}(x+y,t)-u_{N}(x,t)|\,dx \leq 2\int_{|x| > r/4}u_{N}(x,t)\,dx \leq C \exp\left(-r\eta^{-\beta}/C\right),\tag{69}\] where we used \(t \geq \eta\) in the last step. (Note that Proposition 51[uN46conc] requires that \(N>2/t\), which is satisfied since \(N>2/\eta\).) Next, we bound the first term in the left hand side of 68 . Note that for \(x \in \mathbb{R}^{d}\) with \(|x| < r/2\) and since \(|y|<1\), we have \(|x+y| < r\). By Proposition 51[uN46BV], there exists a constant \(C = C(m,d) > 0\) such that \([u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})} \leq Ct^{-d\beta}r^{d-1} \leq C\eta^{-d\beta}r^{d-1}\), so by Proposition 51(i), we conclude that \(u_{N}(\cdot,t) \in \mathop{\mathrm{BV}}(B_{r})\). Therefore, we can approximate \(u_{N}(\cdot,t)\) by a sequence of smooth functions \(\{\varphi^{i}\}_{i \in {\mathbb{N}}} \subset C^{\infty}(B_{r})\) (see, for example, [20]) such that \[\lim_{i\to \infty}\|\varphi^{i}-u_{N}(\cdot,t)\|_{L^{1}(B_{r})} = 0 \text{ and } \lim_{i\to \infty}\|D\varphi^{i}\|_{L^{1}(B_{r})} = [u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})},\] where \(D\varphi\) is the gradient of \(\varphi\). Note that for all \(i \in {\mathbb{N}}\), \[\begin{align} \|\varphi^{i}(\cdot+y)-\varphi^{i}\|_{L^{1}(B_{r/2})} &= \int_{B_{r/2}}\left|\int_{0}^{1}D\varphi^{i}(x+sy)\cdot y\,ds\right|\,dx \\ &\leq |y| \int_{B_{r/2}}\int_{0}^{1}\left|D\varphi^{i}(x+sy)\right|\,ds\,dx \\ &= |y| \int_{0}^{1}\|D\varphi^{i}\|_{L^{1}(B_{r/2}(sy))}\,ds \\ &\leq |y| \cdot \|D\varphi^{i}\|_{L^{1}(B_{r})}, \end{align}\] where in the last step we used that \(B_{r/2}(sy) \subset B_{r}\) because \(|sy| \leq |y| \leq 1 \leq r/2\). Taking \(i \to \infty\) then yields \[\|u_{N}(\cdot+ y,t) - u_{N}(\cdot,t)\|_{L^{1}(B_{r/2})} \leq [u_{N}(\cdot,t)]_{\mathop{\mathrm{TV}}(B_{r})}\cdot |y| \leq C\eta^{-d\beta}r^{d-1}|y|.\] Combining this with 69 , we return to 68 to obtain that for all \(|y| \leq 1\) and \(r \geq 4\), \[\|u_{N}(\cdot + y,t) - u_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})}\leq C\eta^{-d\beta}r^{d-1}|y| + C \exp\left(-r\eta^{-\beta}/C\right).\] Choosing \(r = 4|y|^{-1/d}\) in the above gives \[\|u_{N}(\cdot + y,t) - u_{N}(\cdot,t)\|_{L^{1}(\mathbb{R}^{d})}\leq C\eta^{-d\beta}|y|^{1/d} + C \exp\left(-|y|^{-1/d}\eta^{-\beta}/C\right).\] Because the above bound tends to \(0\) as \(|y| \to 0\), we may define the spatial modulus \(\nu_{\eta}\) as \[\nu_{\eta}(|y|) = \begin{cases} 0 & |y|=0\\ C\eta^{-d\beta}|y|^{1/d} + C \exp\left(-|y|^{-1/d}\eta^{-\beta}/C\right) & 0 < |y| \leq 1\\ \max\left\{C\eta^{-d\beta} + C \exp\left(-\eta^{-\beta}/C\right), 2\right\} &|y|> 1. \end{cases}\] To obtain an approximate temporal modulus of continuity \(\omega_{\eta}\) on \(\mathbb{R}^{d} \times[\eta,T]\), we appeal to Kružkov’s interpolation lemma (Lemma 46) in a manner similar to Lemma 47(iii) albeit only for times in the interval \([\eta,T]\). The only difference is that that proof requires an initial condition \(v_{0} \in L^{\infty}(\mathbb{R}^{d})\) to obtain bounds of the form \[\|v_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})} \leq \|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})} \text{ for } t > 0.\] We can avoid such an assumption for \((u_{N})_{N \geq 2/\eta}\) by using Proposition 51[uN46Linfty] to replace these bounds by bounds of the form \[\|u_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})}\leq Ct^{-d\beta} \leq C\eta^{-d\beta} \text{ for }t \in [\eta,T].\qedhere\] ◻
The preceding lemma allows us to conclude that \((u_{N})_{N \geq 2/\eta}\) satisfies the hypotheses of Lemma 42 on the domain \(\mathbb{R}^{d} \times [\eta,T]\). In Lemma 54, we will show that any \(L^{1}_{\text{loc}}(\mathbb{R}^{d}\times [\eta, T])\)-limit point of this sequence must be a nonnegative entropy solution of the porous medium equation. However, to prove that lemma, we will need the following result.
Lemma 53. Let \(u_{N}\) be generated by \(\mathcal{S}_{N}[A]\) with \(A(r)=r^{m+1}\) and initial measure \(\delta\). Fix \(t > 0\). Assume that there is a subsequence \((u_{N_i})_{i \in {\mathbb{N}}}\) such that \(u_{N_{i}}(\cdot,t) \to w_{t}\) in \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\) for some \(w_{t} \in L^{1}(\mathbb{R}^{d})\). Then, \[\label{e46wunitmass} \int_{\mathbb{R}^{d}}w_{t}(x)\,dx = 1,\qquad{(5)}\] and there exists \(C = C(m,d) > 0\) such that for all \(r > 0\), \[\label{e46wconc} \int_{|x| > r} w_{t}(x)\,dx \leq C\exp\left(-rt^{-\beta}/C\right).\qquad{(6)}\] Finally, we have that \(u_{N_{i}}(\cdot,t) \to w_{t}\) in \(L^{1}(\mathbb{R}^{d})\) (instead of merely in \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\)).
Proof. We remark that \(u_{N_{i}} \geq 0\), and so \(w_{t} \geq 0\) almost everywhere. We first prove ?? . Applying the hypotheses and Proposition 51(i), we have \[\int_{\mathbb{R}^{d}} w_{t}(x) \, dx = \lim_{r\to \infty} \int_{|x| \leq r} w_{t}(x) \, dx = \lim_{r\to \infty} \lim_{i\to\infty} \int_{|x| \leq r} u_{N_{i}}(x,t) \, dx \leq \lim_{r\to \infty} \lim_{i\to\infty} 1 = 1.\] Next, we use Proposition 51 (statements (i) and (iii)) to obtain that for all \(r > 0\), \[\begin{align} \label{e46wbulk} \int_{|x| \leq r} w_{t}(x) \,dx &= \lim_{i\to\infty} \int_{|x| \leq r} u_{N_{i}}(x,t) \, dx \notag\\ &= \lim_{i \to \infty}\left(1 - \int_{|x|> r} u_{N_{i}}(x,t) \, dx \right) \notag\\ &\geq 1 - C\exp(-rt^{-\beta}/C), \end{align}\tag{70}\] where we remark that the hypotheses \(N _{i}> 2/t\) and \(r > 2\sqrt{d}\Delta_x\) are satisfied for all \(N_{i}\) large enough. Taking \(r \to \infty\) in the above gives that \(\int_{\mathbb{R}^{d}} w_{t}(x)\,dx \geq 1\) and so ?? is proved. We note that ?? follows directly from ?? and 70 .
For the convergence in \(L^{1}(\mathbb{R}^{d})\), choose \(r \geq 2\sqrt{d}(2/t)^{-\beta}\) so that \(r \geq 2\sqrt{d}\Delta_x\) for all \(N \geq 2/t\). We combine Proposition 51[uN46conc] and ?? to conclude that for \(N_{i} \geq 2/t\), \[\begin{align} \|u_{N_{i}}(\cdot,t) - w_{t}\|_{L^{1}(\mathbb{R}^{d})} &= \|u_{N_{i}}(\cdot,t) - w_{t}\|_{L^{1}(B_{r})} + \|u_{N_{i}}(\cdot,t) - w_{t}\|_{L^{1}(B^{c}_{r})} \\ &\leq \|u_{N_{i}}(\cdot,t) - u^{\eta}(\cdot,t)\|_{L^{1}(B_{r})} + 2C\exp\left(-rt^{-\beta}/C\right). \end{align}\] Taking \(N_{i}\to \infty\) followed by \(r \to \infty\) in the above gives \(u_{N_{i}}(\cdot,t) \to w_{t}\) in \(L^{1}(\mathbb{R}^{d})\). ◻
Lemma 54. Fix \(\eta \in (0,T)\). Let \(u_{N}\) be generated by \(\mathcal{S}_{N}[A]\) with \(A(r)=r^{m+1}\) and initial measure \(\delta\). There is a subsequence \((u_{N^{\eta}_{n}})_{n \in {\mathbb{N}}}\) and function \(u^{\eta}\) such that \[u_{N^{\eta}_{n}} \xrightarrow[n\to \infty]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times[\eta,T])} u^\eta \text{ and, for all }t \in [\eta,T], u_{N^{\eta}_{n}}(\cdot,t) \xrightarrow[n\to\infty]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})} u^\eta(\cdot,t).\] Furthermore, \(u^{\eta}\) is a nonnegative entropy solution to \(u^{\eta}_{t} - \tfrac{1}{2d}\Delta((u^{\eta})^{m+1}) = 0 \text{ in } \mathbb{R}^{d}\times (\eta,T)\).
Proof. Let \(N_{\eta} \in {\mathbb{N}}\) be such that \(N_{\eta} \geq \frac{2}{\eta}\). Let \(\nu_{\eta}\) and \(\omega_{\eta}\) be respectively a spatial modulus of continuity and an approximate temporal modulus of continuity for \((u_{N})_{N \geq N_{\eta}}\) on \(\mathbb{R}^{d} \times [\eta,T]\), the existence of which is guaranteed by Lemma 52. The existence of these moduli of continuity, along with Proposition 51 (statements (i) and (ii)), entail that \((u_{N})_{N \geq N_{\eta}}\) satisfies the conditions of Lemma 42 on the domain \(\mathbb{R}^{d} \times [\eta,T]\). Therefore, there is a subsequence \((u_{N^{\eta}_{n}})_{n \in {\mathbb{N}}}\) such that \(u_{N^{\eta}_{n}} \to u^{\eta}\) in \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d} \times [\eta,T])\) for some \(u^{\eta} \in L^{1}(\mathbb{R}^{d}\times[\eta,T])\cap L^{\infty}( \mathbb{R}^{d}\times[\eta,T])\cap C([\eta,T];L^{1}(\mathbb{R}^{d}))\). To simplify the notation, we drop the subsequence \((u_{N^{\eta}_{n}})_{n\in{\mathbb{N}}}\) and assume without loss of generality that \(u^{\eta}\) is a limit point of the entire sequence \((u_{N})_{N \geq N_{\eta}}\). The conclusion of Lemma 42 also yields that \(u^{\eta}\) has \(\nu_{\eta}\) and \(\omega_{\eta}\) as a spatial and temporal modulus of continuity, respectively. Hence, we apply Lemma 44 to the sequence \((u_{N})_{N\geq N_{\eta}}\) and the constant sequence \((u^{\eta})_{N \in {\mathbb{N}}}\), deducing that \[\label{e46uNetaslice} \text{for all }t\in [\eta, T], u_{N}(\cdot,t) \xrightarrow{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})}u^{\eta}(\cdot,t).\tag{71}\]
Now we show that \(u^{\eta}\) is a nonnegative entropy solution. By Proposition 51[uN46Linfty], there is a constant \(C = C(m,d) > 0\) such that \[\label{e46uNbdd} \text{for all }t\in [\eta,T], \quad0 \leq u_{N}(\cdot,t) \leq Ct^{-d\beta}.\tag{72}\] The convergence 71 then implies that \[\label{e46uetabdd} \text{for all }t\in [\eta, T], \quad0 \leq u^{\eta}(\cdot,t) \leq Ct^{-d\beta} \text{ a.e.\@ in } \mathbb{R}^{d}.\tag{73}\] Therefore, \(u^{\eta}(\cdot,\eta)\) is nonnegative and belongs to \(L^{\infty}(\mathbb{R}^{d})\), so by Theorem 48 (in particular, the last part of Remark 49), there exists a unique nonnegative entropy solution \(v\) solving \[\label{e46veta} \begin{cases} v_{t} - \frac{1}{2d}\Delta(v^{m+1}) = 0 &\text{in } \mathbb{R}^{d} \times (0,T-\eta) \\ v(\cdot,0) = u^{\eta}(\cdot,\eta) &\text{in } \mathbb{R}^{d}. \end{cases}\tag{74}\] By Remark 41, if we can show that \(u^{\eta}(x,t) = v(x,t-\eta)\) for a.e. \((x,t) \in \mathbb{R}^{d}\times(\eta,T)\), we can conclude that \(u^{\eta}\) is itself a nonnegative entropy solution as desired.
Let \(v_{N}\) be generated by \(\mathcal{S}_{N}\) with initial condition \(u^{\eta}(\cdot,\eta)\). Because of 73 , we can apply the convergence result for diffuse initial conditions, Corollary 50, to obtain that \[\label{e46vNetaslice} v_{N}(\cdot,t) \xrightarrow{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})}v(\cdot,t)\text{ for }t \in [0,T-\eta].\tag{75}\] Since \(u^{\eta}(\cdot,\eta)\) has a spatial modulus of continuity, Lemma 47(iii) implies that \((v_{N})_{N \geq N_{\eta}}\) has an approximate temporal modulus of continuity, possibly after increasing \(N_{\eta}\) depending on \(\|u^{\eta}(\cdot,\eta)\|_{L^{\infty}(\mathbb{R}^{d})}\). Without loss of generality (by Remark 33), we take this approximate temporal modulus of continuity to be \(\omega_{\eta}\).
Next, let \(D \subset \mathbb{R}^{d}\) be compact. For \(t \in [\eta,T]\), we calculate \[\begin{align} &\|u^{\eta}(\cdot,t) - v(\cdot,t-\eta)\|_{L^{1}(D)} \\ &\leq \| (u^{\eta} - u_{N})(\cdot,t)\|_{L^{1}(D)} + \|u_{N}(\cdot,t) - v_{N}(\cdot,t-\eta) \|_{L^{1}(D)} + \|(v_{N} - v)(\cdot,t-\eta)\|_{L^{1}(D)}. \end{align}\] By 71 and 75 , we have \[\label{e46uetav} \|u^{\eta}(\cdot,t) - v(\cdot,t-\eta)\|_{L^{1}(D)} \leq \limsup_{N\to\infty}\|u_{N}(\cdot,t) - v_{N}(\cdot,t-\eta)\|_{L^{1}(D)}.\tag{76}\] To analyze this upper bound, fix \(N \geq N_{\eta}\) and let \(\ell_{N} = \left\lfloor(t-\eta)/\Delta_t\right\rfloor\). Because \(\|v_{0}\|_{L^{\infty}(\mathbb{R}^{d})} = \|u^{\eta}(\cdot,\eta)\|_{L^{\infty}(\mathbb{R}^{d})} \leq C\eta^{-d\beta}\), Lemma 47(i) gives that \(\|v_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})} \leq C\eta^{-d\beta}\) for all \(t \in [0,T-\eta]\). Furthermore, we have that \(\|u_{N}(\cdot,t)\|_{L^{\infty}(\mathbb{R}^{d})} \leq C\eta^{-d\beta}\) by 72 . Hence, by possibly taking \(N_{\eta}\) larger so that \(N \ge N_{\eta}\) satisfies ?? with \(\Lambda := C\eta^{-d\beta}\), we apply Lemma 8(iii) to conclude that \[\begin{align} \tag{77} &\|u_{N}(\cdot,t) - v_{N}(\cdot,t-\eta)\|_{L^{1}(D)} \\ \notag &\leq \|u_{N}(\cdot,t) - v_{N}(\cdot,t-\eta)\|_{L^{1}(\mathbb{R}^{d})} \\\notag &= \|\mathcal{S}^{\ell_{N}}_{N}u_{N}(\cdot - \ell_{N}\Delta_t)- \mathcal{S}^{\ell_{N}}_{N}v_{N}(\cdot, 0)\|_{L^{1}(\mathbb{R}^{d})} \\\notag & \leq \|u_{N}(\cdot, t-\ell_{N}\Delta_t) - v_{N}(\cdot, 0)\|_{L^{1}(\mathbb{R}^{d})} \\\ & \leq \|u_{N}(\cdot, t-\ell_{N}\Delta_t) - u_{N}(\cdot,\eta)\|_{L^{1}(\mathbb{R}^{d})} + \|u_{N}(\cdot,\eta) - v_{N}(\cdot, 0)\|_{L^{1}(\mathbb{R}^{d})}.\tag{78} \end{align}\] For the second term in the upper bound, the fact that \(u_{N}\) and \(v_{N}\) are piecewise constant gives \[\|u_{N}(\cdot,\eta) - v_{N}(\cdot,0)\|_{L^{1}(\mathbb{R}^{d})} = (\Delta_x)^{d} \sum_{k \in \mathbb{Z}^{d}} |u_{N}(k\Delta_x,\eta) - v_{N}(k\Delta_x,0)|.\] Since \(u_{N}\) is piecewise constant and \(v_{N}\) has initial condition \(u^{\eta}(0,\eta)\), we have \[u_{N}(k\Delta_x,\eta) = \frac{1}{|\square_{N}|}\int_{\square_{N}}u_{N}(y+k\Delta_x,\eta)\,dy , \text{and } v_{N}(k\Delta_x,0)=\frac{1}{|\square_{N}|}\int_{\square_{N}}u^{\eta}(y+k\Delta_x,\eta)\,dy.\] Combining the two displays above, we obtain \[\begin{align} &\|u_{N}(\cdot,\eta) - v_{N}(\cdot,0)\|_{L^{1}(\mathbb{R}^d)} \\&= (\Delta_x)^{d} \sum_{k \in \mathbb{Z}^{d}} \left|\frac{1}{|\square_{N}|}\int_{\square_{N}}u_{N}(y+k\Delta_x,\eta)\,dy - \frac{1}{|\square_{N}|}\int_{\square_{N}}u^{\eta}(y+k\Delta_x,\eta)\right| \\&= \sum_{k \in \mathbb{Z}^{d}} \left|\int_{\square_{N}} \bigg(u_{N}(y+k\Delta_x,\eta) - u^{\eta}(y+k\Delta_x,\eta)\bigg)\,dy\right| \\ &\leq \sum_{k \in \mathbb{Z}^{d}} \int_{\square_{N}} \left|u_{N}(y+k\Delta_x,\eta) - u^{\eta}(y+k\Delta_x,\eta)\right| \,dy\\ &= \int_{\mathbb{R}^{d}} \left|u_{N}(y,\eta) - u^{\eta}(y,\eta)\right| \,dy \to 0, \end{align}\] where in the last step, we use the final statement of Lemma 53 to bootstrap the convergence \(u_{N}(\cdot,\eta) \to u^{\eta}(\cdot,\eta)\) in \(L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})\) to convergence in \(L^{1}(\mathbb{R}^{d})\).
For the first term in 78 , we use \(\omega_{\eta}\), an approximate temporal modulus of continuity for \((u_{N})_{N\geq\eta}\) on \(\mathbb{R}^{d}\times[\eta,T]\), to obtain \[\|u_{N}(\cdot,t-\ell_{N}\Delta_t) - u_{N}(\cdot,\eta)\|_{L^{1}(\mathbb{R}^{d})} \leq \omega_{\eta}(|t-\ell_{N}\Delta_t- \eta| + \tfrac{1}{N}) \xrightarrow{N \to \infty} 0,\] where we used that \(\ell_{N}\Delta_t= \left\lfloor(t-\eta)/\Delta_t\right\rfloor\Delta_t\xrightarrow{N \to \infty} (t-\eta)\). Therefore, combining the previous two displays, we return to 76 to obtain \[\|u^{\eta}(\cdot,t) - v(\cdot,t-\eta)\|_{L^{1}(D)} = 0 \text{ for all }t \in [\eta,T].\] Since \(D \subset \mathbb{R}^{d}\) was arbitrary, \(u^{\eta}(x,t) = v(x,t-\eta)\) for a.e. \((x,t) \in \mathbb{R}^{d}\times(\eta,T)\). Thus we conclude that \(u^{\eta}\) is a nonnegative entropy solution of the porous medium equation with initial condition \(\delta\). ◻
We now present a convergence result for \((u_{N})_{N>0}\) satisfying a finite difference scheme with initial measure \(\delta\), which converges to the Barenblatt solution of the porous media equation.
Theorem 55. Let \(u_{N}\) be generated by \(\mathcal{S}_{N}[A]\) with \(A(r)=r^{m+1}\) and initial measure \(\delta\). We recall that the Barenblatt solution \(\bar{u}\) is given by \(\bar{u}(x,t):=t^{-d\beta}(C-\gamma|x|^{2}t^{-2\beta})_{+}^{\frac{1}{m}}.\) Then \[u_{N} \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})} \bar{u} \text{ and, for all }t \in (0,T], u_{N}(\cdot,t) \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})} \bar{u}(\cdot,t).\]
Proof. In this proof, we frequently work with restrictions of the functions \(u_N\) to a subdomain of the form \(\mathbb{R}\times I\) for some interval \(I\). We abuse notation by continuing to refer to such restrictions as \(u_N\), rather than writing \(u_N|_{\mathbb{R}\times I}\). Now that this convention has been pointed out, it should cause no confusion.
Fix any increasing sequence of positive integers \((M_i)_{i \ge 1}\). We first use a diagonalization argument to show that there exists a subsequence \((N_i)_{i \in{\mathbb{N}}}\) of \((M_i)_{i \in {\mathbb{N}}}\) such that \[\label{e46utildeconv} u_{N_{i}} \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})} \tilde{u} \text{ and, for all }t \in (0,T], u_{N_{i}}(\cdot,t) \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})} \tilde{u}(\cdot,t),\tag{79}\] where \(\tilde{u} \in L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})\) is a distributional solution to \(\tilde{u}_{t} - \frac{1}{2d}\Delta(\tilde{u}^{m+1}) = 0\). To this end, fix a decreasing sequence \((\eta_{i})_{i\in{\mathbb{N}}} \subset (0,T)\) with \(\lim_{i\to\infty}\eta_{i} = 0\). By applying Lemma 54 for each \(\eta_{i}\), we have that, for each \(i \in {\mathbb{N}}\), there exists an increasing sequence \((N^{\eta_{i}}_{j})_{j \in {\mathbb{N}}} \subset {\mathbb{N}}\) such that, as \(j \to \infty\), \[u_{N^{\eta_{i}}_{j}} \xrightarrow{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times(\eta_{i},T))} u^{\eta_{i}} \text{ and, for all }t \in [\eta_{i},T], u_{N^{\eta_{i}}_{j}}(\cdot,t) \xrightarrow{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})} u^{\eta_{i}}(\cdot,t),\] where \(u^{\eta_{i}}\) is an entropy solution to \(u^{\eta_{i}}_{t} - \frac{1}{2d}\Delta((u^{\eta_{i}})^{m+1}) = 0\) in \(\mathbb{R}^{d}\times(\eta_{i},T)\). Furthermore, these subsequences may be constructed iteratively so that \((N^{\eta_{i+1}}_{j})_{j \in {\mathbb{N}}}\) is a subsequence of \((N^{\eta_{i}}_{j})_{j \in {\mathbb{N}}}\) for all \(i \in {\mathbb{N}}\). It follows that for all \(i \in {\mathbb{N}}\), \[u_{N^{\eta_{i+1}}_{j}} \xrightarrow[j\to\infty]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times(\eta_{i},T))}u^{\eta_{i}}\quad\text{ and }\quad u_{N^{\eta_{i+1}}_{j}} \xrightarrow[j\to\infty]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d}\times(\eta_{i+1},T))}u^{\eta_{i+1}} .\] This means that \[\label{e46domainex} u^{\eta_{i+1}} \overset{a.e.}{=} u^{\eta_{i}}\text{ in }\mathbb{R}^{d} \times (\eta_{i},T).\tag{80}\] In other words, \(u^{\eta_{i+1}}\) extends \(u^{\eta_{i}}\) to the larger domain \(\mathbb{R}^{d}\times(\eta_{i+1},T)\) (up to a set of measure zero). Next, we define \(\tilde{u}: \mathbb{R}^{d} \times (0,T]\to \mathbb{R}\) as the a.e. limit of these domain extensions, meaning \[\tilde{u}(x,t) := \begin{cases} u^{\eta_{0}}(x,t) &\text{ if } \eta_{0} \leq t \\ u^{\eta_{i}}(x,t) &\text{ for } t \in [\eta_{i+1},\eta_{i}), i \in {\mathbb{N}}. \end{cases}\]
We now show that \(\tilde{u} \in C((0,T];L^{1}(\mathbb{R}^{d}))\). Because \(u^{\eta_{i}} \in C([\eta_{i},T];L^{1}(\mathbb{R}^{d}))\) for every \(i \in {\mathbb{N}}\), we combine 80 with Corollary 45 to conclude that for all \(i \in {\mathbb{N}}\), \(t \geq \eta_{i}\) and \(j \geq i\), \(u^{\eta_{j}}(\cdot,t) \overset{a.e.}{=} u^{\eta_{i}}(\cdot,t)\). Thus, for all \(i \in {\mathbb{N}}\), and \(t \geq \eta_{i}\), \(\tilde{u}(\cdot,t) \overset{a.e.}{=} u^{\eta_{i}}(\cdot,t)\), and so \(\tilde{u} \in C([\eta_{i},T];L^{1}(\mathbb{R}^{d}))\). Therefore, because \(\eta_{i}\to 0\), \(\tilde{u} \in C((0,T];L^{1}(\mathbb{R}^{d}))\).
Next, note that for all \(i \in {\mathbb{N}}\), using 80 and the definition of \(\tilde{u}\), we have that \(\tilde{u} \overset{a.e.}= u^{\eta_{i}}\) in \(\mathbb{R}^{d} \times (\eta_{i},T)\). Therefore, for all \(i \in {\mathbb{N}}\), \(\tilde{u}\) is an entropy solution of the porous medium equation in \(\mathbb{R}^{d} \times (\eta_{i},T)\), which means, by Proposition 39 that for all \(i \in {\mathbb{N}}\), \(\tilde{u}\) is a distributional solution in \(\mathbb{R}^{d} \times (\eta_{i},T)\). Hence, because \(\eta_{i} \to 0\), \(\tilde{u}\) is a distributional solution in \(Q_{T}\). Finally, setting \(N_{i}:=N^{\eta_{i}}_{i}\), the sequence of functions \((u_{N_i})_{i \in {\mathbb{N}}}\) then satisfies 79 .
Next, we show that \(\tilde{u}\) is a.e. equal to the Barenblatt solution \(\bar{u}\). Let \(\varphi\in C_{c}(\mathbb{R}^{d})\). Because \(\varphi\) is compactly supported and continuous, it is uniformly continuous and thus admits a modulus of continuity, which we denote by \(\rho\). Fix \(t \in (0,T]\) and \(\varepsilon> 0\). By Lemma 53, \[\int_{\mathbb{R}^{d}} \tilde{u}(x,t) \, dx = 1 \quad \text{ and }\quad \int_{|x| > \varepsilon} \tilde{u}(x,t) \,dx \leq C\exp(-\varepsilon t^{-\beta}/C).\] This implies \[\begin{align} \left|\int_{\mathbb{R}^{d}}\tilde{u}(x,t)\varphi(x)\,dx - \varphi(0) \right|&= \left|\int_{\mathbb{R}^{d}}\tilde{u}(x,t)(\varphi(x)-\varphi(0))\,dx \right| \\ &\leq \int_{|x| \leq \varepsilon}\tilde{u}(x,t)|\varphi(x)-\varphi(0)|\,dx + \int_{|x| > \varepsilon}\tilde{u}(x,t)|\varphi(x)-\varphi(0)|\,dx \\ &\leq \rho(\varepsilon) \int_{|x| \leq \varepsilon}\tilde{u}(x,t)\,dx + 2 \|\varphi\|_{L^{\infty}(\mathbb{R}^{d})} \int_{|x| > \varepsilon}\tilde{u}(x,t)\,dx \\ &\leq \rho(\varepsilon) + 2 \|\varphi\|_{L^{\infty}(\mathbb{R}^{d})} C\exp(-\varepsilon t^{-\beta}/C). \end{align}\] Taking \(t \to 0^{+}\), followed by \(\varepsilon\to 0^{+}\) in the above display gives \[\lim_{t\to0^{+}}\int_{\mathbb{R}^{d}}\tilde{u}(x,t)\varphi(x)\,dx = \varphi(0),\] and hence \(\tilde{u}\) has initial trace \(\delta\). Therefore, by the uniqueness of distributional solutions (Theorem 37), \(\tilde{u} = \bar{u}\) a.e. in \(\mathbb{R}^{d} \times (0,T)\).
To conclude that the two solutions are a.e. equal on a fixed time slice, note that earlier in the proof, we showed \(\tilde{u} \in C((0,T];L^{1}(\mathbb{R}^{d}))\). It is straightforward to use the definition of \(\bar{u}\) in 23 to see that that \(\bar{u} \in C((0,T];L^{1}(\mathbb{R}^{d}))\), so by Corollary 45, it follows that for \(t \in (0,T]\), \(\tilde{u}(\cdot,t) = \bar{u}(\cdot,t)\) a.e. in \(\mathbb{R}^{d}\). Hence, we can re-write 79 as \[u_{N_{i}} \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(Q_{T})} \bar{u} \text{ and, for all }t \in (0,T], u_{N_{i}}(\cdot,t) \xrightarrow[]{L^{1}_{\mathop{\mathrm{loc}}}(\mathbb{R}^{d})} \bar{u}(\cdot,t).\] Thus, for any increasing sequence \((M_i)_{i \in {\mathbb{N}}}\) there exists a further subsequence \((N_i)_{i \in {\mathbb{N}}}\) along which the above convergences both hold; the result follows. ◻
We are now ready to prove Theorem 1
Proof of Theorem 1. For \(N \in {\mathbb{N}}\) let \(u_N\) be generated by \({\mathcal{S}}_N[A]\) with \(A(r)=r^{m+1}\) and initial condition \(\delta\). Choosing any \(T \geq 1\), by Theorem 55 we have that \(u_{N}(\cdot,1) \xrightarrow{L^{1}_{\text{loc}}(\mathbb{R}^{d})} \bar{u}(\cdot,1)\).
Now we show convergence in distribution. Let \(D \subset \mathbb{R}^{d}\) be a continuity set, meaning \(|\partial D|=0\), and take \(N \geq 2\). Since \(u_{N}(k\Delta_x,n\Delta_t) = |\square_{N}|^{-1}{\mathbf{P}}\left\{X^{n} = k\right\}\), \[\begin{align} {\mathbf{P}}\left\{\frac{1}{N^{1/(dm+2)}}X^{N} \in D\right\} &= {\mathbf{P}}\left\{\Delta_xX^{N} \in D\right\} \\ &=\sum_{k\Delta_x\in (D \cap \mathbb{Z}^{d}\Delta_x)}{\mathbf{P}}\left\{X^{N}= k\right\} \\ &=\sum_{k\Delta_x\in (D \cap \mathbb{Z}^{d}\Delta_x)} u_{N}(k\Delta_x,1) |\square_{N}|, \end{align}\] where in the last step we used that \(|\square_{N}| = (\Delta_x)^{d}\) and \(N \Delta_t= 1\). To write this last term as an integral of \(u_{N}\) over \(D\), we need to account for the discretization of the domain. Define \[D_{N} := \bigcup_{\square_{N}(k\Delta_x) \subset D}\square_{N}(k\Delta_x).\] Continuing from our previous calculation, we have \[{\mathbf{P}}\left\{\frac{1}{N^{1/(dm+2)}}X^{N} \in D\right\} =\sum_{k\Delta_x\in D \cap \mathbb{Z}^{d}\Delta_x} u_{N}(k\Delta_x,1) |\square_{N}| =\int_{D_{N}}u_{N}(x,1)\,dx.\] On the other hand, by the definition of the random variable \(B\), \[{\mathbf{P}}\left\{B \in D\right\} = \int_{D}\bar{u}(x,1)\,dx.\] Combining the above two displays, this implies \[\begin{align} &\left| {\mathbf{P}}\left\{\frac{1}{N^{1/(dm+2)}}X^{N} \in D\right\} - {\mathbf{P}}\left\{B \in D\right\}\right| \\ &= \left| \int_{D_{N}}u_{N}(x,1)\,dx - \int_{D}\bar{u}(x,1)\,dx\right| \\ &\leq \left| \int_{D_{N}}u_{N}(x,1)\,dx - \int_{D}u_{N}(x,1)\,dx\right| + \left| \int_{D}u_{N}(x,1)\,dx - \int_{D}\bar{u}(x,1)\,dx\right|. \end{align}\] For the latter term in the upper bound, since \(u_{N}(\cdot,1) \xrightarrow[N\to\infty]{L^{1}_{\text{loc}}(\mathbb{R}^{d})} \bar{u}(\cdot,1)\), \[\left| \int_{D}u_{N}(x,1)\,dx - \int_{D}\bar{u}(x,1)\,dx\right| \xrightarrow[N\to \infty]{} 0.\] For the other term, for \(N \geq 2\), by taking \(t = 1\) in Proposition 51[uN46Linfty], we have that \(\|u_{N}(\cdot,1)\|_{L^{\infty}(\mathbb{R}^{d})} \leq C\) and so \[\left| \int_{D_{N}}u_{N}(x,1)\,dx - \int_{D}u_{N}(x,1)\,dx\right| = \left|\int_{D\setminus D_{N}}u_{N}(x,1)\,dx\right| \leq C |D \setminus D_{N}|.\] Since \(\limsup_{N\to\infty}|D\setminus D_{N}| = 0\), we combine the previous three displays to conclude that \[{\mathbf{P}}\left\{\frac{1}{N^{1/(dm+2)}}X^{N} \in D\right\} \xrightarrow[N\to\infty]{} {\mathbf{P}}\left\{B \in D\right\}\, ,\] which implies that \(N^{-1/(dm+2)}X^{N} \rightarrow B\) in distribution. ◻
In this section, we consider properties of \(b\)-lazy random walks. Let \(Y_n\) be a \(b\)-lazy symmetric random walk in \(d\) dimensions started from initial distribution \(h(\cdot)=\boldsymbol{1}_{0}(\cdot)\) (i.e. started from the origin). Let \(q^{(b)}_n(k) = {\mathbf{P}}\left\{Y_n = k\right\}\).
For the convenience of the reader, we recall that \(T(R,b)\) as in 27 is given by \[T(R, b) := \min\left\{n \ge 0: \text{there exists } k \in \mathbb{Z}^d \text{ with }|k| > R\text{ and }\Delta q^{(b)}_n(k) < 0\right\}.\] In particular, since \(q^{(b)}_{n+1} = q^{(b)}_n + \frac{b}{2d}\Delta q^{(b)}_n\), where \(\Delta q^{(b)}_n(k) = \sum_{\ell\sim k} (q^{(b)}_n(\ell) - q^{(b)}_n(k))\) is the discrete Laplacian, we see that \[\Delta q_n^{(b)} = {q^{(b)}_{n+1} - q^{(b)}_n \over b/2d},\] so \(T(R, b)\) can be interpreted as the first time \(n\) where for some \(|k|>R\), the sequence \(({\mathbf{P}}\left\{Y_{n}=k\right\})_{n\geq 0}\) decreases in time.
We begin by proving a related statement about a non-lazy random walk in \(d\) dimensions, which we will later relate to lazy random walks. Let \(\left\{\bar{Y}_{n}\right\}\) be the simple, symmetric random walk on \(\mathbb{Z}^{d}\) started at the origin. That is, \(\bar{Y}_0 = 0\), and \(\bar{Y}_{n+1} - \bar{Y}_n\) is chosen uniformly and independently from \(\{\pm e_{i}\}_{i=1}^{d}\).
In this case, it does not make sense to compute \(T(R,b)\) for \(\bar{Y}\), because \({\mathbf{P}}\left\{\bar{Y}_{n}=k\right\}=0\) whenever \(n + \sum_{i=1}^{d} k_i\) is odd. Nevertheless, we are able to compare \({\mathbf{P}}\left\{\bar{Y}_n = k\right\}\) and \({\mathbf{P}}\left\{\bar{Y}_{n-2} = k\right\}\).
Theorem 56. Let \(\bar{Y}_n\) be as above. There is a constant \(\Lambda=\Lambda(d) > 0\) such that, if \(2 \le n \le \Lambda|k|^2\), then \[\left(1 + {1 \over n}\right){\mathbf{P}}\left\{\bar{Y}_{n-2} = k\right\} \le {\mathbf{P}}\left\{\bar{Y}_n = k\right\}.\]
In order to prove Theorem 56, we require a technical lemma which we first state (and delay its proof until after the proof of Theorem 56).
Lemma 57. Suppose \(k, m \in \mathbb{Z}^d\) and \(|k_i| \le m_i\) with \(\sum_{i=1}^{d} m_i = n-2\). Let \(\Lambda:= (8d^4)^{-1}\). If \(2 \le n \le \Lambda|k|^2\), then \[{n(n-1) \over d^3} \sum_{i=1}^{d} {1 \over ((m_i+2)^2 - k_i^2)} \ge 1 + {1 \over n}.\]
Equipped with Lemma 57, we now present the proof of Theorem 56.
Proof of Theorem 56. Suppose we are given a path \((\bar{Y}_0, \ldots, \bar{Y}_n)\in (\mathbb{Z}^{d})^{n}\). Let \(M(n) \in \mathbb{Z}^d\) denote the move vector of the path up to time \(n\), whose \(i\)th-coordinate is given by \[M(n)_i = \#\{0 \le j < n: \bar{Y}_{j+1} - \bar{Y}_j = \pm e_i\}.\] Observe that for each \(i=1,\ldots, d\), \(M(n)_i\) is the number of times that the \(i\)-th coordinate has changed, up to time \(n\).
For \(k,m\in \mathbb{Z}^{d}\) and \(n\in {\mathbb{N}}\), let \(P_n(k; m)\) be the probability that \(\bar{Y}_n = k\) and \(M(n) = m\). These probabilities have an exact formula under certain hypotheses on \(m\): if \[\label{e46movec} \begin{cases} \sum_{i=1}^{d} m_i = n,\\ \text{m_i \ge |k_i|, for i=1, \ldots, d},\\ \text{m_i+k_i is even for i=1,\ldots,d}, \end{cases}\tag{81}\] then \[P_n(k; m) = \left(\begin{gather} n\\[-.2em] {\displaystyle {m_1 + k_1 \over 2}, {m_1 - k_1 \over 2}, \ldots, {m_d + k_d \over 2}, {m_d - k_d \over 2}} \end{gather}\right) (2d)^{-n},\] where \(\genfrac{(}{)}{0pt}{}{n}{a,\,b,\,c, \ldots}\) denotes the multinomial coefficient. If any of those three conditions in 81 fail, then the probability \(P_n(k;m)\) is zero.
Given \(k,m \in \mathbb{Z}^d\), if \(P_{n-2}(k;m)>0\), then for any \(i\in \left\{1, \ldots, d\right\}\), \(P_{n}(k;m+2e_i)>0\), and the above exact formula yields the identity \[\begin{align} \label{eq:pnidentity} P_{n-2}(k; m) &= {\displaystyle 4d^2 \left({m_i + 2 + k_i \over 2}\right) \left({m_i + 2 - k_i \over 2}\right) \over n(n-1)} P_n(k; m + 2e_i) \nonumber\\ &= {d^2 \over n(n-1)} ((m_i + 2)^2 - k_i^2) P_n(k; m + 2e_i).\nonumber \end{align}\tag{82}\] Rearranging the above expression and taking an average over \(i = 1, \ldots, d\), we obtain that for any valid vector \(m\) for a path of length \(n-2\), \[\left[{n(n-1) \over d^3}\sum_{i=1}^{d} {1 \over ((m_i+2)^2 - k_i^2)}\right] P_{n-2}(k; m) = {1 \over d} \sum_{i=1}^{d} P_n(k; m + 2e_i).\]
By Lemma 57, for \(\Lambda= (8d^4)^{-1}\), since \(2 \le n \le \Lambda|k|^2\) by hypothesis, we conclude \[\left(1 + {1 \over n}\right) P_{n-2}(k; m) \le {1 \over d} \sum_{i=1}^{d} P_n(k; m + 2e_i).\] Summing over \(m\in \mathbb{Z}^{d}\) such that \(P_{n-2}(k,m)>0\), we obtain \[\left(1 + {1 \over n}\right) \sum_{m:P_{n-2}(k,m)>0} P_{n-2}(k; m) \le {1 \over d} \sum_{m:P_{n-2}(k,m)>0} \sum_{i=1}^{d} P_n(k; m + 2e_i).\] The left side is \((1+1/n) {\mathbf{P}}\left\{\bar{Y}_{n-2} = k\right\}\), and each move vector \(m'\) with \(\sum_{i=1}^{d} m'_i = n\) can be written as a sum \(m + 2e_i\) in at most \(d\) ways, so the right side is no greater than \(\sum_{m'} P_n(k; m') = {\mathbf{P}}\left\{\bar{Y}_n = k\right\}\). This proves the theorem. ◻
We now return to the proof of Lemma 57.
Proof of Lemma 57. For ease of notation, let \(y_i = m_i+2\). We begin by factoring \[\label{e46factor}\sum_{i=1}^d {1 \over y_i^2 - k_i^2} = \sum_{i=1}^d {1 \over y_i^2} + \sum_{i=1}^d {k_i^2 \over (y_i^2-k_i^2)y_i^2}.\tag{83}\] We estimate each term in the right hand side from below. Let \(\mu := d^{-1} \sum_{i=1}^{d} y_i\). We apply Jensen’s inequality with the function \(f(x) = 1/x^2\): \[\sum_{i=1}^{d} {1 \over y_i^2} = d \left({1 \over d} \sum_{i=1}^{d} {1 \over y_i^2}\right) \ge {d \over \mu^2} = {d^3 \over (\sum_{i=1}^{d} y_i)^2}.\]
Since \(\sum_{i=1}^{d}m_{i}=n-2\), \(\sum_{i=1}^{d} y_i=n+2d-2\), so\[\begin{align} {n(n-1) \over d^3} \sum_{i=1}^{d} {1 \over y_i^2} &\ge {n(n-1) \over (\sum_{i=1}^{d} y_i)^2} \notag \\&= {n(n-1) \over (n+2d-2)^2} \notag \\&= \left(1-{1 \over n}\right)\left(1+{2d-2 \over n}\right)^{-2}. \notag \end{align}\] Then, since \((1+(2d-2)/n)^{-2} \ge (1-(2d-2)/n)^{2}\geq 1-(4d-4)/n\), we have \[{n(n-1) \over d^3} \sum_{i=1}^{d} {1 \over y_i^2} \ge \left(1-\frac{1}{n}\right)\left(1-\frac{4d-4}{n}\right) \ge 1 - {4d-3 \over n}.\]
We estimate the second term in 83 in the following way. Since \(\sum_{i=1}^{d} m_i=n - 2\), for each \(i=1, \ldots, d\), \(y_i = m_i + 2 \le n\). Moreover, \(k_i^2/(y_i^2 - k_i^2)y_i^2\) is at least \(k_i^2/y_i^4\). Therefore\[\begin{align} {n(n-1) \over d^3} \sum_{i=1}^{d} {k_i^2 \over (y_i^2 - k_i^2)y_i^2} &\ge {n(n-1) \over d^3} \sum_{i=1}^{d} {k_i^2 \over y_i^4}. \notag\\&\ge {n(n-1) \over d^3 n^4} \sum_{i=1}^{d} k_i^2 \notag\\&\ge{1\over 2d^3n^2} |k|^2\label{simple46estimb} \end{align}\tag{84}\] where in the final line, we used the estimate \(n(n-1) \ge 1/2n^2\) because \(n \ge 2\). Our assumption is that \(n \le \Lambda|k|^2\), so the estimate in (84 ) is bounded from below by \(1/2\Lambda d^3 n = 4d/n\). Combining this with the prior display, we obtain \[{n(n-1) \over d^3} \sum_{i=1}^{d} {1 \over y_i^2 - k_i^2} \ge 1 - {4d-3 \over n} + {4d \over n} = 1 + {3 \over n}.\]This proves the lemma. ◻
Before returning back to the lazy random walk, we first prove a preparatory lemma which tells us the asymptotic behaviour of \(q_n^{(1/2)}(k)\) when \(n = \lfloor |k|^2 /16d^4 \rfloor\) and \(k\to \infty\).
Recall that \(q^{(1/2)}_n(k) = \mathbb{P}\left\{X_1 + \cdots + X_n = k\right\}\) is the probability distribution at step \(n\) of a \(\frac{1}{2}\)-lazy random walk in \(\mathbb{Z}^d\). Since \(\mathbb{E}[X_1]\) is the zero vector and the covariance matrix is \(\text{Cov}[X_1] = \text{Id}/2d\), the central limit theorem yields that \((X_1 + \cdots + X_n) / \sqrt{n} \to_d N(0, \text{Id}/2d)\).
However, we will require a sharper version of this convergence. By a result of Bhattacharya and Ranga Rao [21], it follows that \[\label{weightlowerbound46a}\sup_{k \in \mathbb{Z}^d} (1 + |k|^2)\left|q^{(1/2)}_n(k) - \varphi_n(k)\right| = o(n^{-d/2})\tag{85}\] where \(\varphi_n(k) := (d / \pi n)^{d/2}e^{-d|k|^2/n}\) is the continuous probability density of \(N(0, n\text{Id}/2d)\).
(Note: we only need the leading order, so in the notation of [21], we set \(s = 2\). Also note that the definition on page 52 of [21] says \(\widetilde{P}_0 \equiv 0\), but in fact one should set \(\widetilde{P}_0 \equiv 1\), and \(P_0(-\phi; \{\chi_\nu\})\) is then the standard normal distribution.)
We are now ready to state the precise bound on \(q_{n}^{(1/2)}\).
Lemma 58. Let \(\eta > 0\). There are positive constants \(k_{1}=k_{1}(\eta, d)\), \(a=a(\eta, d)\) such that for any \(k\in \mathbb{Z}^d\) with \(|k| \ge k_{1}\), \[q_n^{(1/2)}(k) \ge \frac{a}{n^{d/2}} \qquad \text{where } n := \lfloor |k|^2\eta^{-1}\rfloor.\]
Proof. Let \(\varepsilon_n\) be the scaled maximum difference between the two functions \(q_n^{(1/2)}\) and \(\varphi_n\) over lattice points in \(\mathbb{Z}^d\), i.e. \[\varepsilon_n := n^{d/2} \sup_{k\in \mathbb{Z}^d} \left|q_n^{(1/2)}(k) - \varphi_n(k)\right|.\] The supremum here is bounded above by the supremum in (85 ), so \(\varepsilon_n\) vanishes as \(n \to \infty\).
Let \(a := (1/2) (d/\pi)^{d/2} e^{-2d\eta}\). Let \(n_0\) be the smallest positive integer so that \(\varepsilon_n \le a\) for \(n \ge n_0\). Such an integer exists because \(\varepsilon_n \to 0\). Let \(k_1: = \sqrt{2\eta n_0}\) so that \(k_{1}^{2}\eta^{-1}=2n_{0}\).
Suppose \(|k| \ge k_{1}\). We first observe that, for any \(\alpha\geq 1\), then \(\lfloor \alpha\rfloor \ge \alpha/2\). Thus for \(|k|\geq k_{1}\), \(|k|^2\eta^{-1} \ge k_{1}^2\eta^{-1} = 2n_0 \ge 1\), so by definition \(n = \lfloor |k|^2\eta^{-1} \rfloor \ge |k|^2 (2\eta)^{-1}\).
We conclude that for \(n= \lfloor |k|^2\eta^{-1} \rfloor\), \(n\geq |k|^2(2\eta)^{-1} \ge k_{1}^2 (2\eta)^{-1}= n_0\), and thus \(\varepsilon_n\le{a}\). Furthermore, since \(n \ge |k|^2(2\eta)^{-1}\), this implies \(d|k|^2/n \le 2d\eta\), and hence, \[\varphi_n(k) = \left(d \over \pi n\right)^{d/2} e^{-d|k|^2/n} \ge \left(d \over \pi n\right)^{d/2} e^{-2d\eta} = {2a \over n^{d/2}}\]
The definition of the error \(\varepsilon_n\) implies \(|q_n^{(1/2)}(k) - \varphi_n(k)| \le \varepsilon_n/n^{d/2}\), and thus \(q_n^{(1/2)}(k) \ge \varphi_n(k) - \varepsilon_{n}/n^{d/2}\). Combine this with the upper bound on \(\varepsilon_n\) and the lower bound \(\varphi_n(k)\), we obtain \[\label{weightlowerbound46b} q_n^{(1/2)}(k) \ge \varphi_n(k) - {\varepsilon_n \over n^{d/2}} \ge \varphi_n(k) - {a \over n^{d/2}} \ge {a \over n^{d/2}}.\tag{86}\] ◻
We now convert two-step information about a non-lazy random walk \(\bar{Y}_{n}\) into one-step information about a 1/2-lazy random walk \(Y_{n}\).
Lemma 59. If \(|k| \ge 3\) and \(1 \le n \le \Lambda|k|^2\) for \(\Lambda=\Lambda(d)\) as in Theorem 56, then \[\left(1 + {1 \over 8n}\right)q^{(1/2)}_{n-1}(k) \le q^{(1/2)}_n(k).\]
Proof. Throughout this proof, the point \(k\) is fixed, so we suppress it from the notation whenever there is no ambiguity. Let \(\omega_1, \omega_2, \ldots\) be a sequence of IID \(\text{Bernoulli}(1/2)\)-distributed \(\left\{0,1\right\}\)-valued random variables. Then \(q_n^{(1/2)}\) can be interpreted as an expectation of the non-lazy (simple) random walk \(q^{(1)}_{\cdot}\) at a random time: \[\begin{align} q^{(1/2)}_n &= {\mathbf{E}}\left[q^{(1)}_{\omega_1 + \cdots + \omega_n}\right]. \end{align}\] If \(n=1,2\), then \(q^{(1/2)}_{n-1}(k)\) is zero because \(|k| \ge 3\), so the conclusion of the lemma is vacuously true. If \(n \ge 2\), then \(\omega_1 + \omega_2 = 0,1,2\) with respective probabilities \(1/4, 1/2, 1/4\), so \[\begin{align} q^{(1/2)}_n &= \frac{1}{4} {\mathbf{E}}\left[q^{(1)}_{\omega_3 + \cdots + \omega_n} + 2q^{(1)}_{1 + \omega_3 + \cdots + \omega_n} + q^{(1)}_{2 + \omega_3 + \cdots + \omega_n}\right]\notag \\&= \frac{1}{4} {\mathbf{E}}\left[{\widehat q}_{2+\omega_3 + \cdots + \omega_n}\right] \end{align}\] where \({\widehat q}_n := q^{(1)}_n + 2q^{(1)}_{n-1} + q^{(1)}_{n-2}\). The value of this depends on parity:\[{\widehat q}_n(k) = \begin{cases}q^{(1)}_n(k) + q^{(1)}_{n-2}(k)&\text{ if }n+\sum k_i\text{ is even}\\2q^{(1)}_{n-1}(k)&\text{ if }n+\sum k_i\text{ is odd.}\end{cases}\]
If \(3 \le n \le \Lambda|k|^2\), then Theorem 56 holds for both \(n\) and \(n-1\): \[q_n^{(1)} \ge \left(1 + {1 \over n}\right)q_{n-2}^{(1)} \qquad q_{n-1}^{(1)} \ge \left(1 + {1 \over n-1}\right)q_{n-3}^{(1)} \ge \left(1 + {1 \over n}\right) q_{n-3}^{(1)}.\] If \(n + \sum k_i\) is even, then \((n-1) + \sum k_i\) is odd, so \[\begin{align} {\widehat q}_n &= q^{(1)}_n + q^{(1)}_{n-2} \\&\ge \Big(1+\frac{1}{n}+1\Big) q^{(1)}_{n-2} \ge \Big(1 + \frac{1}{2n}\Big) {\widehat q}_{n-1}. \end{align}\] If \(n + \sum k_i\) is odd, then by similar reasoning, \[\begin{align} {\widehat q}_n &= 2q^{(1)}_{n-1} \\&= \Big(1 + \frac{1}{4n}\Big) q^{(1)}_{n-1} + \Big(1-\frac{1}{4n}\Big) q^{(1)}_{n-1} \\&\ge \Big(1 + \frac{1}{4n}\Big) q^{(1)}_{n-1} + \Big(1-\frac{1}{4n}\Big)\Big(1+\frac{1}{n}\Big) q^{(1)}_{n-3} \\&\ge\Big(1 + \frac{1}{4n}\Big)(q^{(1)}_{n-1} + q^{(1)}_{n-3})\\&=\Big(1 + \frac{1}{4n}\Big) {\widehat q}_{n-1}, \end{align}\] where in the fourth line, we used the estimate that since \(n\geq 1\), \((1-(4n)^{-1}) (1+n^{-1}) = 1 + 3(4n)^{-1} - (4n^2)^{-1} \ge 1+(2n)^{-1}\).
In both cases, we get the inequality \((1+(4n)^{-1}){\widehat q}_{n-1} \le {\widehat q}_n\), and thus, since \(2+\omega_{3}\cdots+\omega_{n-1}\leq n-1\leq n\), we have \[\begin{align} \Big(1+\frac{1}{4n}\Big) {\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}}\right] &\leq \frac{1}{4}\Big(1+\frac{1}{4(2 + \omega_3 + \cdots + \omega_{n-1})}\Big) {\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}}\right]\\ &\leq {\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}+1}\right]\\ &=2{\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}+\omega_{n}}\right]-{\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}}\right]. \end{align}\] We arranging and multiplying by \(1/4\), we obtain \[\frac{1}{4}\Big(2+\frac{1}{4n}\Big) {\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}}\right]\leq \frac{2}{4}{\mathbf{E}}\left[{\widehat q}_{2 + \omega_3 + \cdots + \omega_{n-1}+1}\right],\] and hence \[\Big(2+\frac{1}{4n}\Big)q_{n-1}^{(1/2)}\leq 2q_{n}^{(1/2)},\] which implies the result. 0◻
Finally, we are ready to prove Theorem 17. Recall that we aim to show that there are constants \(k_2\) such that , if the lazy parameter \(b\leq 1/8\), then for \(|k| \ge k_2\) and \(n \le \Lambda|k|^2/6b\) for \(\Lambda\) as in Theorem 56, \[q^{(b)}_n(k) \le q^{(b)}_{n+1}(k).\]
Proof of Theorem 17. Let \(\nu_1, \nu_2, \ldots\) be independent \(\left\{0,1\right\}\)-valued random variables that are \(\text{Bernoulli}(2b)\)-distributed. Consider the following process on \(\mathbb{Z}^{d}\). Starting from the origin, at step \(n\), if \(\nu_n = 1\), then we take a \(1/2\)-lazy random walk step, i.e. with probability \(1/2\), we take a unit step in one of the \(2d\) directions, or with probability \(1/2\), we stay where we are. If \(\nu_n = 0\), we stay put.
On the one hand, this is just a \(b\)-lazy random walk, because we jump to a uniformly chosen neighbour with probability \(b\) at each step. On the other hand, at the \(n\)-th step, we have taken \(\nu_1 + \cdots + \nu_n\) steps in a \(1/2\)-lazy random walk. Consequently, \[q_n^{(b)}(k) = \mathbb{E}\left[q_{\nu_1 + \cdots + \nu_n}^{(1/2)}(k)\right].\] We may equivalently express this as \[q^{(b)}_n(k) = \sum_{m=0}^\infty q^{(1/2)}_m(k) \,\mathbb{P}\{\nu_1 + \cdots + \nu_n = m\}.\] Let \(\delta q_j^{(1/2)}(k):= q^{(1/2)}_{j+1}(k) - q^{(1/2)}_j(k)\). Then since \(|k|\geq k_{2}\) to be chosen, by a telescoping series, we have \[\begin{align} \sum_{m=0}^\infty q^{(1/2)}_m(k) \mathbb{P}\{\nu_1 + \cdots + \nu_n = m\}&=\sum_{m=0}^{\infty} \sum_{j =0}^{m-1} \delta q^{(1/2)}_j(k) \mathbb{P}\{\nu_1 + \cdots + \nu_n = m\} \\&=\sum_{j=0}^{\infty} \delta q^{(1/2)}_j(k)\sum_{m=j+1}^{\infty} \mathbb{P}\{\nu_1 + \cdots + \nu_n = m\} \\&=\sum_{j=0}^{\infty} \delta q_j ^{(1/2)}(k)\mathbb{P}\{\nu_1 + \cdots + \nu_n \ge j+1\}. \end{align}\] That means that the difference of successive probabilities is \[\begin{align} q^{(b)}_{n+1}(k) - q^{(b)}_n(k) &= \sum_{j=0}^{\infty} \delta q_j^{(1/2)}(k) \big(\mathbb{P}\{\nu_1 + \cdots + \nu_{n+1} \ge j+1\} - \mathbb{P}\{\nu_1 + \cdots + \nu_n \ge j+1\}\big) \\&= \sum_{j=0}^{\infty} \delta q_j^{(1/2)}(k)\mathbb{P}\{\nu_1 + \cdots + \nu_n = j, \nu_{n+1} = 1\} \\&= 2b \sum_{j=0}^{\infty} \delta q_j^{(1/2)}(k) \mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}. \end{align}\]This is a weighted sum of the differences \(\delta q_j^{(1/2)}(k)\). By Lemma 59, if \(j + 1 \le \Lambda|k|^2\), then \[\delta q^{(1/2)}_j (k)\geq{1 \over 8(j+1)} q_j^{(1/2)}(k) \ge {1 \over 8\Lambda|k|^2} q_j^{(1/2)}(k).\]
Applying this lower bound to the prior display, for the indices \(j = 0, \ldots, \lfloor \Lambda|k|^2 \rfloor - 1\), we obtain \[\begin{align}[t]\label{lowb} q^{(b)}_{n+1}(k) - q^{(b)}_n(k) &\ge {b \over 4\Lambda|k|^2} \sum_{j=0}^{\lfloor \Lambda|k|^2 \rfloor - 1} q^{(1/2)}_j(k) \,\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}\\&\qquad+2b\sum_{j=\lfloor \Lambda|k|^2 \rfloor}^\infty \delta q_j^{(1/2)}(k) \,\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}\\ &=: S_{1}+S_{2}.\end{align}\tag{87}\] We want to show that the right hand side is nonnegative. The rough idea is that \(\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}\) should decrease very quickly as \(j\) increases when \(j\) is much larger than \(\mathbb{E}[\nu_1 + \cdots + \nu_n] = 2bn \le \Lambda|k|^2/3\).
It turns out that we get exponential decay if \(j \ge \Lambda|k|^2/2\), as we now show. The probabilities in (87 ) have a simple formula, \(\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\} = (2b)^j (1-2b)^{n-j} \genfrac{(}{)}{0pt}{}{n}{j}\). In particular, the ratio of consecutive probabilities is \[{\mathbb{P}\{\nu_1 + \cdots + \nu_n = j+1\} \over \mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}} = {\genfrac{(}{)}{0pt}{}{n}{j+1} (2b)^{j+1} (1-2b)^{n-j-1} \over \genfrac{(}{)}{0pt}{}{n}{j} (2b)^j (1-2b)^{n-j}} = {2b(n-j) \over (1-2b)(j+1)}.\] If \(j + 1 \ge \Lambda|k|^2 / 2\), then since by assumption \(n \le \Lambda|k|^2 / 6b\) and \(b \le 1/8\), then \[{2b(n-j) \over (1-2b)(j+1)} \le {2bn \over (3/4) (\Lambda|k|^2/2)} \le \frac{\Lambda |k|^{2}}{3}\frac{4}{3}\frac{2}{\Lambda |k|^{2}}= {8 \over 9},\] which implies that \[{\mathbb{P}\{\nu_1 + \cdots + \nu_n = j+1\} \over \mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}}\leq \frac{8}{9}.\] We now iterate this estimate. Let \(\gamma:= \lfloor \Lambda|k|^2 / 2 \rfloor\). If \(j \ge \gamma\), then \[\label{inc46chain}\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\} \le (8/9) \mathbb{P}\{\nu_1 + \cdots + \nu_{n} = j-1\} \le \cdots \le (8/9)^{j-\gamma} \rho\tag{88}\] where \(\rho := \mathbb{P}\{\nu_1 + \cdots + \nu_n = \gamma\}\).
We will use this to compare \(|S_{2}|\) with \(S_{1}\). Let \(a, k_1\) be the constants from Lemma 58 with \(\eta=\Lambda^{-1}\). Let \(k_2\geq \max\{1, 4/\Lambda, k_1\}\), and sufficiently large so that, for \(c\) to be chosen, \[\label{ak0bound} {a \over 4\Lambda^{1+d/2} |k|^{2+d}} \ge c\left(\frac{8}{9}\right)^{\tfrac{\Lambda|k|^2}{2}}\qquad \text{ for }|k| \ge k_2.\tag{89}\] This is possible because the right-hand side decreases exponentially, while the left-hand side only decreases polynomially.
The term with index \(\gamma\) is part of the first sum, because \(\gamma\le \Lambda|k|^2/2 \le \lfloor \Lambda|k|^2 \rfloor\).2 Every term in the first sum is nonnegative, so \(S_1\) is at least equal to the \(\gamma\) term. Then by an application of Lemma 58, and the choice of constants, we have \[\begin{align} S_1&\ge {b \over 4\Lambda|k|^2} q_{\gamma}^{(1/2)}(k) \,\rho \ge {ab \over 4\Lambda|k|^2 \gamma^{d/2}} \,\rho\ge {ab \over 4\Lambda^{1+d/2} |k|^{2 +d}} \,\rho.\label{s1bound}{} \end{align}\tag{90}\]
On the other hand, for \(|S_{2}|\), we claim there exists an absolute constant \(c\) such that, by (88 ), \[\begin{align} \label{s2bound} |S_2| &\le 2b\sum_{j=\lfloor \Lambda|k|^2 \rfloor}^\infty \delta q_j^{(1/2)}(k)\mathbb{P}\{\nu_1 + \cdots + \nu_n = j\}\le 4b\sum_{j=\lfloor \Lambda|k|^2 \rfloor}^\infty (\tfrac{8}{9})^{j-\gamma}\rho\le cb(\tfrac{8}{9})^{\Lambda|k|^2/2}\rho. \end{align}\tag{91}\] The first term of the sum is \((8/9)^{\lfloor \Lambda|k|^2 \rfloor - \lfloor \Lambda|k|^2/2 \rfloor} \rho\), so \(c = 4\times 9 \times (9/8)\) would make the inequality true, for example.
By (89 ), the lower bound (90 ) is larger than the upper bound (91 ), so \[q^{(b)}_{n+1}(k) - q^{(b)}_n \ge S_1 + S_2 \ge S_{1}-|S_{2}|\geq 0.\] Therefore \(q^{(b)}_n(k) \le q^{(b)}_{n+1}(k)\) as long as \(n \le \Lambda|k|^2/6b\). ◻
LAB acknowledges support from the NSERC Discovery Grants program and from the Canada Research Chairs program. This material is based in part upon work supported by the National Science Foundation under Grant No. DMS-1928930, while LAB was in residence at the Simons Laufer Mathematical Sciences Institute in Berkeley, California, during the semester of Spring 2025. GB from the NSERC Alexander Graham Bell Canada Graduate Scholarship. JL acknowledges support from NSERC Discovery Grant 2018-06371 and 2025-05575, and the Canada Research Chairs program 2018-00154 and 2023-00081.