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Chapters 5 and 6: The Keller-Segel system in self-similar variables

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Chapters 5 and 6 are a joint work with J. Dolbeault. They are devoted to the study of the parabolic-elliptic Keller-Segel model

which describes the motion of unicellular amoebae, like dictyostelium discoideum. Here u denotes their spatial density and it makes sense to consider them in a two-dimensional setting. A straightforward computation (see [109, pages 122–124] and [122]) shows that solutions (with second moment initially finite) blow-up in finite time if the total mass is large enough (larger than 8⇡ with our conventions), while, for solutions with smaller masses, the diffusion dominates the large time asymptotics.

More precisely, it has been shown in [100, 72, 66, 88], that if n0 2L1+⇣ then there exists a solution u, in the sense of distributions, that is global in time and such that M = R

R3u(x, t) dx is preserved along the evolution. There is no non-trivial stationary solution to (2.3.1) and any solution converges to zero locally as time gets large. It is therefore convenient to study the asymptotic behavior of u in self-similar variables, where space and time scales are given respectively by R(t) :=p In this variables the system can be written as

8>

Existence of a stationary solution to (2.3.3) has been established in [76] by ODE techniques, and in [107]

by PDE methods. This stationary solution is unique according to [79]. Moreover it has been shown in [66]

that nand rc converge ast! 1, respectively in L1(R2) and L2(R2) to this unique stationary solution which involves smooth and radially symmetric functions.

A simple computation of the second moment shows that smooth solutions with mass larger than 8⇡ blow-up in finite time; see for instance [100]. The case M = 8⇡ has been extensively studied. We shall refer to [79, 80, 81] for some recent papers on this topic. The asymptotic regime is of a very different nature in such a critical case. In the chapters 5 and 6 we shall restrict our purpose to the sub-critical case M <8⇡.

The rate of convergence towards the stationary solution in self-similar variables gives, after undoing the change of variables, the rate of convergence towards the asymptotic profile for the solutions of (2.3.1).

In [65], it has been proved that ifM is less than some massM 2(0,8⇡), then convergence holds at an exponential rate, which is essentially governed by the linearization of System (2.3.3) around the stationary

solution. However, the estimate of the value ofM was found to be significantly smaller than 8⇡. In the radially symmetric setting, V. Calvez and J.A. Carrillo have found in [67] that the rate measured with respect to Wasserstein’s distance does not depend on the mass, in the whole range (0,8⇡). The goal of chapters 5 and 6 is to prove a similar estimate with no symmetry assumption.

In chapter 5 we define a proper functional framework and prove a functional inequality which is the crucial tool for obtaining the main result of chapter 6. Let us describe briefly this framework. InR2 the logarithmic Hardy-Littlewood-Sobolev has been established with optimal constants in [69] (also see [64]) and can be written as

Z

R3n dx. Equivalently, inequality (2.3.4) can be written as Z equivalent to the euclidian Onofri’s inequality.

To study the Keller-Segel system written in self-similar variables, equation (2.3.3), it turns out to be convenient to use an equivalent form of the logarithmic Hardy-Littlewood-Sobolev inequality, which, provided that M <8⇡, can be written as

Z where (nM, cM) denotes the unique stationary solution, of (2.3.3), given by

−∆cM =M e12|x|2+cM R

R3e12|x|2+c dx =:nM , x2R2 .

Following [69, 64, 68, 71], we show by duality that (2.3.5) corresponds to a new Onofri type inequality.

Theorem 4 For everyM 2(0,8⇡), and for all function φsmooth and compactly supported, one has log functional associated with the inequality around φ⌘1. By density, it is possible to attain an inequality in the functional space obtained when the set of smooth functions with compact support is completed with respect to the normkφk2 =R

R3|rφ|2 dx+ (R

R2φ dµM)2. This is the main result of chapter 5.

The inequality obtained by expanding aroundφ= 1 is a Poincar´e type inequality. It has a counterpart in the Hardy-Littlewood-Sobolev framework, which can be written as

Q1[f] :=

This suggests to write the linearized Keller-Segel system on the space of square integrable functions with respect todµM, which are orthogonal to the one-dimensional kernel of the linearized operatorL, endowed

CHAPTER 2. INTRODUCTION (ENGLISH VERSION) 23 with the scalar product associated to the quadratic form Q1. ThenL is self-adjoint and we prove that it has an explicit spectral gap:

Q1[f] =hf, fi  hf, Lfi=:Q2[f].

Details onL and in particular on its spectrum are given later. With these preliminaries in hand, one can then study the large time asymptotics of the solutions to the Keller-Segel system and relate the spectral gap with rates of convergence.

In chapter 6 we provide refined asymptotics concerning the large-time behavior of the solutions of the two-dimensional Keller-Segel system in self-similar variables. It has been shown in [65] that there exists a positive massM? 8⇡ such that for any initial datan02L2(nM1dx) of massM < M? satisfying (2.3.2), System (2.3.3) has a unique solution nsuch that

Z

R2|n(t, x)−nM(x)|2 dx

nM(x) C e2δ t 8t≥0

for some positive constants C and δ. Moreover δ can be taken arbitrarily close to 1 as M ! 0. If M <8⇡, we may notice that the condition n0 2L2(nM1dx) is stronger than (2.3.2). Our main result is that M? = 8⇡ and δ = 1, at least for a large subclass of solutions with initial datum n0 satisfying the following technical assumption

9"2(0,8⇡−M) such that Z s

0

n0,(σ)dσ Z

B 0,p

s/⇡nM+"(x)dx 8s≥0. (2.3.6)

Theorem 5 Assume thatn0 satisfies the technical assumption (2.3.6), n0 2L2+(nM1dx) and M :=

Z

R3

n0dx <8⇡ . Then any solution of (2.3.3) with initial datum n0 is such that

Z

R2|n(t, x)−nM(x)|2 dx

nM(x) C e2t 8t≥0

for some positive constant C, where nM is the unique stationary solution to (2.3)with mass M.

This result turns out to be consistent with the recent results of [67] for the two-dimensional radial model and its one-dimensional counterpart. The estimateδ= 1 is sharp. For completeness, let us mention that results of exponential convergence for problems with mean field have been obtained earlier in [89, 90], but only for interaction potentials involving much smoother kernels than G2.

To obtain this result, we establish uniform estimates on knkLp(R2) by applying symmetrization tech-niques as in [93, 94], and then prove the uniform convergence ofntonM using Duhamel’s formula. Our main tool are the spectral gap of the linearized operator L and the strict positivity of the linearized entropy in the appropriate functional space.

2.4 Chapters 7 and 8: A numerical study and a matched asymptotics

Dans le document The DART-Europe E-theses Portal (Page 32-35)