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Sharp macroscopic blow-up behavior for the parabolic-elliptic Keller-Segel system in dimensions $n\ge 3$

Loth Damagui Chabi, Philippe Souplet

TL;DR

The paper provides a sharp macroscopic description of finite-time blow-up for the parabolic-elliptic Keller-Segel system in dimensions $3\le n\le 9$ with radially decreasing data. It proves the existence of nonflat backward self-similar profiles $U\in\mathcal S\setminus\{1\}$ and shows that solutions satisfy $u(x,t)=(1+o(1))\frac{1}{T-t}U\left(\frac{|x|}{\sqrt{T-t}}\right)$ as $(x,t)\to(0,T)$, together with a two-sided bound $\frac{C_1}{T-t+|x|^2}\le u(x,t)\le\frac{C_2}{T-t+|x|^2}$ in a neighborhood of blow-up and a sharp final profile $u(x,T)\sim L|x|^{-2}$ with $L>0$. The work extends to type I and time-monotone solutions, refines known estimates, and provides a streamlined, robust proof strategy based on the averaged mass, similarity variables, and zero-number arguments to yield the macroscopic concentration behavior in the original space-time variables. These results significantly sharpen the understanding of chemotactic blow-up by delivering macroscopic-scale asymptotics and a precise final blow-up profile, complementing prior microscopic descriptions.

Abstract

We study the space-time concentration or blow-up asymptotics of radially decreasing solutions of the parabolic-elliptic Keller-Segel system in the whole space or in a ball. We show that, for any solution in dimensions $3\le n\le 9$ (assuming finite mass in the whole space case), there exists a nonflat backward self-similar solution $U$ such that $$u(x,t)=(1+o(1))U(x,t),\quad\hbox{as $(x,t)\to (0,T)$.}$$ This macroscopic behavior is important from the physical point of view, since it gives a sharp description of the concentration phenomenon in the scale of the original space-time variables~$(x,t)$. It strongly improves on existing results, since such behavior was previously known (\cite{GMS}) to hold only in the microscopic scale $|x|\le O(\sqrt{T-t})$ as $t\to T$ (and in the whole space case only). As a consequence, we obtain the two-sided global estimate $$C_1\le (T-t+|x|^2)u(x,t)\le C_2\quad\hbox{in $B_R\times(T/2,T)$},$$ whose upper part only was known before (\cite{Soup-Win}), as well as the sharp final profile: $$\lim_{x\to 0} |x|^2u(x,T)=L\in(0,\infty).$$ The latter improves, with a different proof, the recent result of \cite{BZ} by excluding the possibility $L=0$. We also give extensions of these results, in higher dimensions, to type~I and to time monotone solutions. Moreover, we extend the known results on type I estimates and on convergence in similarity variables, and significantly simplify their proofs.

Sharp macroscopic blow-up behavior for the parabolic-elliptic Keller-Segel system in dimensions $n\ge 3$

TL;DR

The paper provides a sharp macroscopic description of finite-time blow-up for the parabolic-elliptic Keller-Segel system in dimensions with radially decreasing data. It proves the existence of nonflat backward self-similar profiles and shows that solutions satisfy as , together with a two-sided bound in a neighborhood of blow-up and a sharp final profile with . The work extends to type I and time-monotone solutions, refines known estimates, and provides a streamlined, robust proof strategy based on the averaged mass, similarity variables, and zero-number arguments to yield the macroscopic concentration behavior in the original space-time variables. These results significantly sharpen the understanding of chemotactic blow-up by delivering macroscopic-scale asymptotics and a precise final blow-up profile, complementing prior microscopic descriptions.

Abstract

We study the space-time concentration or blow-up asymptotics of radially decreasing solutions of the parabolic-elliptic Keller-Segel system in the whole space or in a ball. We show that, for any solution in dimensions (assuming finite mass in the whole space case), there exists a nonflat backward self-similar solution such that This macroscopic behavior is important from the physical point of view, since it gives a sharp description of the concentration phenomenon in the scale of the original space-time variables~. It strongly improves on existing results, since such behavior was previously known (\cite{GMS}) to hold only in the microscopic scale as (and in the whole space case only). As a consequence, we obtain the two-sided global estimate whose upper part only was known before (\cite{Soup-Win}), as well as the sharp final profile: The latter improves, with a different proof, the recent result of \cite{BZ} by excluding the possibility . We also give extensions of these results, in higher dimensions, to type~I and to time monotone solutions. Moreover, we extend the known results on type I estimates and on convergence in similarity variables, and significantly simplify their proofs.
Paper Structure (12 sections, 21 theorems, 140 equations)

This paper contains 12 sections, 21 theorems, 140 equations.

Key Result

Theorem 2.1

Let $3\le n\le 9$ and consider problem 0 with $\Omega=\mathbb{R}^n$ or $\Omega=B_R$. Assume that $u_0$ satisfies i0, along with $u_0\in L^1(\mathbb{R}^n)$ in case $\Omega=\mathbb{R}^n$, and that $T=T(u_0)<\infty$.

Theorems & Definitions (43)

  • Theorem 2.1
  • Remark 2.1
  • Theorem 2.2
  • Proposition 2.3
  • Theorem 2.4
  • Corollary 2.5
  • Remark 3.1
  • Remark 3.2
  • Proposition 4.1
  • Remark 4.1
  • ...and 33 more