Evolution Driven by the Infinity Fractional Laplacian Félix del TesoJørgen EndalyEspen R. JakobsenzJuan Luis Vázquezx October 13 2022

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Evolution Driven by the Infinity Fractional Laplacian
Félix del Teso?Jørgen EndalEspen R. JakobsenJuan Luis Vázquez§
October 13, 2022
Abstract
We consider the evolution problem associated to the infinity fractional Laplacian introduced by
Bjorland, Caffarelli and Figalli (2012) as the infinitesimal generator of a non-Brownian tug-of-war
game. We first construct a class of viscosity solutions of the initial-value problem for bounded
and uniformly continuous data. An important result is the equivalence of the nonlinear operator
in higher dimensions with the one-dimensional fractional Laplacian when it is applied to radially
symmetric and monotone functions. Thanks to this and a comparison theorem between classical
and viscosity solutions, we are able to establish a global Harnack inequality that, in particular,
explains the long-time behavior of the solutions.
Keywords: Fractional partial differential equations, infinity fractional Laplacian, infinity Laplacian,
viscosity solutions.
2020 Mathematics Subject Classification. 35R11, 35K55, 35A01, 35B45.
Contents
1 Introduction 2
2 Preliminaries and statement of main results 3
3 Properties of a approximation scheme 7
4 Definitions, existence and properties of viscosity solutions 12
5 Review of basic results on the fractional heat equation 16
6 Smooth solutions and the 1d fractional heat equation 17
7 Comparison and local truncation errors 20
8 Global Harnack principle 22
9 Extensions and open problems 23
?Departamento de Matemáticas, Universidad Autónoma de Madrid. felix.delteso@uam.es
Department of Mathematical Sciences, Norwegian University of Science and Technology. jorgen.endal@ntnu.no
Department of Mathematical Sciences, Norwegian University of Science and Technology. espen.jakobsen@ntnu.no
§Departamento de Matemáticas, Universidad Autónoma de Madrid. juanluis.vazquez@uam.es
1
arXiv:2210.06414v1 [math.AP] 12 Oct 2022
1 Introduction
In this paper we study a parabolic equation associated to the (normalized) infinity fractional Laplacian
operator. We recall that the local version of the game had been introduced by Peres et al. in 2009
([31]) where it is shown that the standard infinity Laplace equation is solved by the value function for
a two-players random turn “tug–of–war” game. The game is as follows: a token is initially placed at a
position x0and every turn a fair coin is tossed to choose which of the players plays. This player
moves the token to any point in the ball of radius ε > 0around the current position. If, eventually,
iterating this process, the token reaches a point xe, the players are awarded (or penalized) f(xe)
(payoff function). For a PDE overview of the infinity Laplacian operator and its role as an absolute
minimizer for the Lnorm of the gradient, see [24,25].
In 2012 Bjorland, Caffarelli and Figalli ([5]) introduced equations involving the so-called infinity
fractional Laplacian as a model for a nonlocal version of the “tug-of-war” game. Following their
explantation, instead of flipping a coin at every step, every player chooses a direction and it is an
s-stable Lévy process that chooses both the active player and the distance to travel. The infinity
fractional Laplacian, with symbol s
, is a nonlinear integro-differential operator, the original definition
is given in Lemma 2.1 below. However, for the purpose of this paper, we also consider the alternative
equivalent definition introduced in [5] (see also [14]) given by
s
φ(x) := Cssup
|y|=1
inf
|˜y|=1 ˆ
0
(φ(x+ηy) + φ(xη˜y)2φ(x)) dη
η1+2swhere s(1/2,1). (1.1)
The constant is usually taken as Cs= (4ssΓ(1
2+s))/(π1
2Γ(1 s)) but the value is irrelevant for our
results. In their paper [5] the authors study two stationary problems involving the infinity fractional
Laplacian posed in bounded space domains, namely, a Dirichlet problem and a double-obstacle problem.
Here, we consider the evolution problem
(tu(x, t)=∆s
u(x, t), x Rn, t > 0,
u(x, 0) = u0(x), x Rn,
(1.2)
(1.3)
with s(1/2,1) and n2. When n= 1 the operator s
is just the usual linear fractional Laplacian
operator (∆)sof order s, and equation (1.2) is just the well-known fractional heat equation [6,21].
See also a detailed study of that equation using PDE techniques in [18,3,7,36]. Note that for n2
the operator is nonlinear so a new theory is needed. A non-normalized version is introduced in [10]
along with a well-posedness theory for the corresponding equations of the type (1.2)–(1.3). However,
the two problems are not equivalent nor closely related.
Here we develop an existence theory of suitable viscosity solutions for the parabolic problem (1.2)–
(1.3), based on approximation with monotone schemes. We show that the obtained class of solutions
enjoys a number of good properties. As in the elliptic case [5], we lack a uniqueness result in the
context of viscosity solutions. However, we are able to prove an important comparison theorem relat-
ing two types of solutions, classical and viscosity ones, see Theorem 2.6. As a counterpart, we also
obtain uniqueness and comparison of classical solutions. Moreover, we show that for smooth, radially
symmetric functions and nonincreasing along the radius in Rnwith n2, the operator s
reduces
to the classical fractional Laplacian (∆)sin dimension n= 1 (Theorem 6.1). A similar example
regarding nondecreasing one-dimensional profiles can be found in Lemma 6.3. In this way we may con-
struct a large class of classical solutions that make the comparison theorem relevant (Theorems 2.10
and 2.12). Note that no similar reduction applies in general, even in the radial case (see Subsection
6.2 for a counterexample).
Using the developed tools, we study the asymptotic behavior of the constructed solutions, and obtain
a global Harnack type principle, see Theorem 2.13.
2
1.1 Related literature
It is interesting to compare the nonlocal model (1.2) with the local version of the infinity Laplacian
that has been studied by many authors, both in the stationary and evolution cases, cf. [2,19,24,1,31,
32,33,25]. Asymptotic expansions for the game theoretical p-Laplacian in the local case and related
approximation schemes in the elliptic case are studied in [27,28,17] and in the parabolic case in [26].
For the variational version of the p-Laplacian operator see [15].
There exist in the literature other nonlocal generalizations of the p-Laplacian and the infinity Lapla-
cian. Let us mention (i) the normalized version [5,4] with asymptotic expansions and game theoretical
approach [8,14,23]; (ii) nonnormalized version [10] both elliptic and parabolic; (iii) Hölder infinity
Laplacian [9]; and (iv) the (variational) fractional p-Laplacian [12,29,35,30,34,11,37].
2 Preliminaries and statement of main results
First let us fix some notation that we will use along the paper.
For given δ > 0, standard mollifiers are denoted by ρδ. Following [5], we say that φC1,1(x)at some
xRnif there exists pxRnand Cx, ηx>0such that
|φ(x+y)φ(x)px·y| ≤ Cx|y|2for all |y|< ηx. (2.1)
Note that C2
b(BR(x)) C1,1(x). Here Ck
b(U)is the space of functions on the set Uwith bounded
continuous derivatives of all orders in [0, k]. Let us also define:
B(Rn) := {φ:RnR|φis pointwisely bounded},
UC(Rn) := {φ:RnR|φis uniformly continuous},
BU C(Rn) := B(Rn)UC(Rn)with kφkCb(Rn):= sup
xRn|φ(x)|,
and for β(0,1], we define |φ|C0(Rn)= supx,yRn|φ(x)φ(y)|/|xy|βand
C0(Rn) := {φCb(Rn)|kφkC0<∞} where kφkC0=kφkCb+|φ|C0.
A modulus of continuity is a nondecreasing function ω:R+R+such that limr0+ω(r) = 0. For a
function fBU C(Rn), we define the corresponding modulus of continuity as follows:
ωf(r) = sup
|y|≤rkf(·+y)fkCb(Rn).
For a Hölder continuous function fC0(Rn),ωf(r)≤ |f|C0rβ.
We will also need ei:= (0,0,...,0,1,0,...,0) Rn, where 1is at the ith component.
2.1 Alternative characterization of the infinity fractional Laplacian
We have the following alternative characterization of operator s
that we will use throughout:
Lemma 2.1 (Alternative characterization).Assume φC1,1(x)B(Rn). Then:
If φ(x)6= 0, then
s
φ(x) = Csˆ
0φ(x+ηζ) + φ(xηζ)2φ(x)dη
η1+2swhere ζ:= φ(x)/|∇φ(x)|.
3
If φ(x)=0, then
s
φ(x) = Cssup
|y|=1 ˆ
0φ(x+ηy)φ(x)dη
η1+2s+Csinf
|y|=1 ˆ
0φ(xηy)φ(x)dη
η1+2s.
The equivalence when φ(x)=0follows from the fact that the integrals in this case are well-defined
and can be combined to get (1.1). When φ(x)6= 0, it can be shown that the supremum and infimum
of (1.1) is actually taken at ζ, see Proposition 2.2 in [14]. To sketch the proof, assume for simplicity
that the supremum in (1.1) is taken at y, and let us argue that y=ζ. Indeed, by splitting the integral
and using the definitions of C1,1and the infimum,
s
φ(x)Csˆ
0φ(x+ηy) + φ(xηζ)2φ(x)dη
η1+2sCsφ(x)·(yζ)ˆηx
0
ηdη
η1+2s+C.
Now, since s
φ(x)is well-defined and the integral diverges if y6=ζ, we must have y=ζ. A similar
argument holds for the infimum.
2.2 Existence of solutions and basic properties
We are able to construct a suitable class of viscosity solutions of (1.2)–(1.3). The two steps are as
follows:
(i) Approximating s
by removing the singularity, i.e., we introduce
Lε[φ](x) := Cssup
|y|=1
inf
|˜y|=1 ˆ
εφ(x+ηy) + φ(xη˜y)2φ(x)dη
η1+2s.
(ii) Discretizing in time by letting τ > 0and tj:= jτ for jN, i.e., tjτN, and then considering
the semidiscrete problem
Uj+1(x)Uj(x)
τ=Lε[Uj](x), x Rn, j N,
U0(x) = u0(x), x Rn.
(2.2)
(2.3)
We study the properties of (2.2)–(2.3) in Section 3. Existence of viscosity solutions follows by taking
the limit in this approximate scheme, as well as properties inherited from the approximations.
Theorem 2.2 (Existence and a priori results).If u0BU C(Rn), then there is at least one viscosity
solution uCb(Rn×[0,)) of (1.2)(1.3). Moreover:
(a) (Cb-bound) For all t > 0,ku(·, t)kCb(Rn)≤ ku0kCb(Rn).
(b) (Uniform continuity in space) For all yRnand all t > 0,
ku(·+y, t)u(·, t)kCb(Rn)ωu0(|y|).
(c) (Uniform continuity in time) For all t, ˜
t > 0,
ku(·, t)u(·,˜
t)kCb(Rn)˜ω(|t˜
t|)where ˜ω(r) := infδ>0nωu0(δ) + rsupε>0kLε[u0]kCb(Rn)o
is a modulus satisfying ˜ω(r)ωu0(r1/3) + Cr1/3+r,C:= csku0kCb(Rn)k∇ρk22s
L1(Rn)kD2ρk2s1
L1(Rn),
and ρis a standard mollifier.
Remark 2.3. The definition of viscosity solutions is given Section 4(Definition 4.3). We obtain
viscosity solution as limits of monotone approximations of the problem in Section 3.
4
Note that if u0is Hölder continuous and s(1/2,1), then the above modulii will be (more) explicit.
Lemma 2.4. If u0C0(Rn)for β(0,1], then
ωu0(δ) = |u0|C0δβand kLε[u0]kCb(Rn)c(s, ρ)|u0|C0δβ2s.
The above result will be proved at the end of Section 4.
It follows after a minimization in δthat ˜ω(r) = c(s, ρ)|u0|C0r1
2s, and the solution uwill be Hölder
continuous with the correct parabolic regularity.
Corollary 2.5 (Existence and a priori results).If u0C0 (Rn)for β(0,1], then there is at least
one viscosity solution uCb(Rn×[0,)) of (1.2)(1.3). Moreover:
(a) (Cb-bound) For all t > 0ku(·, t)kCb(Rn)≤ ku0kCb(Rn).
(b) (Hölder in space) For all yRnand all t > 0,
ku(·+y, t)u(·, t)kCb(Rn)≤ |u0|C0|y|β.
(c) (Hölder in time) There is a constant c(s, ρ)only depending on sand ρsuch that for all t, ˜
t > 0,
ku(·, t)u(·,˜
t)kCb(Rn)C|u0|C0|t˜
t|β
2s.
2.3 Classical solutions, radial solutions, comparison, and uniqueness
There could be other ways of obtaining viscosity solutions, and unfortunately, we lack general com-
parison and uniqueness results. Nevertheless, we can obtain that classical solutions are unique and we
can compare our constructed viscosity solutions with classical sub- and supersolutions of (1.2)–(1.3).1
Theorem 2.6 (Comparison between classical and viscosity solutions).Assume u0BUC(Rn).
Let u, u C2
b(Rn×[0,)) be respective classical sub- and supersolution of (1.2)(1.3), and let
uBU C(Rn×[0,)be a viscosity solution of (1.2)(1.3)as constructed in Theorem 2.2. Then
uuuin Rn×(0,).
The above result is proved in Section 7. We want to emphasize that it is done in a rather nonstandard
way, since we inherit the comparison from the approximation scheme when the solution is classical. In
general, this cannot be done in the context of viscosity solutions since the approximation scheme only
converges up to a subsequence.
Remark 2.7. By Theorem 2.6, we can in addition get comparison of constructed viscosity solutions
as long as the initial datas are separated by an initial data which produces a classical solution.
An immediate consequence of Theorem 2.6:
Corollary 2.8 (Comparison of classical sub- and supersolutions).Let u, v C2
b(Rn×[0,)) be
respective classical sub- and supersolutions of (1.2)(1.3)with initial data u0, v0. If u0v0, then
uv.
Corollary 2.9 (Uniqueness of solutions).Classical solutions of (1.2)(1.3)in C2
b(Rn×[0,)) are
unique.
Theorem 2.6 might be an empty statement unless we provide a class of classical solutions of (1.2)–(1.3).
The following result, proved in Section 6, solves this issue.
1We will work with classical solutions in C2
b. Actually, we can reduce to C1
bfor the temporal variable, and to C1,1B
for the spatial variables.
5
摘要:

EvolutionDrivenbytheInnityFractionalLaplacianFélixdelTeso?JørgenEndalyEspenR.JakobsenzJuanLuisVázquezxOctober13,2022AbstractWeconsidertheevolutionproblemassociatedtotheinnityfractionalLaplacianintroducedbyBjorland,CaarelliandFigalli(2012)astheinnitesimalgeneratorofanon-Browniantug-of-wargame.We...

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