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Existence of finite time blow-up in Keller-Segel system

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arxiv 2312.01475 v1 pith:QRYVHCV3 submitted 2023-12-03 math.AP

classification math.AP
keywords fracmathbblambdastarbeginblow-upcasescdot
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abstract

Perhaps the most classical diffusion model for chemotaxis is the Keller-Segel system $\begin{equation} \begin{cases} u_{t} =\Delta u - \nabla \cdot(u \nabla v) \ \ \ \text{in } \mathbb{R}^2\times(0,T),\\[5pt] v = (-\Delta_{\mathbb{R}^2})^{-1} u := \displaystyle\frac {1}{2\pi} \displaystyle\int_{\mathbb{R}^2} \log \frac {1}{|x-z|}u(z,t) dz, \ \ \ \ \ \ \ \ \ (\star)\\[5pt] u(\cdot ,0) = u_{0}^{\star} \ge 0 \ \ \ \text{in } \mathbb{R}^2. \end{cases} \end{equation}$ We show that there exists $\varepsilon>0$ such that for any $m$ satisfying $8\pi<m\le 8\pi+\varepsilon$ and any $k$ given points $q_{1},...,q_{k}$ in $\mathbb{R}^{2}$ there is an initial data $u_0^*$ of $(\star)$ for which the solution $u(x,t)$ blows-up in finite time as $t\to T$ with the approximate profile $$u(x,t)=\sum_{j=1}^{k}\frac{1}{\lambda_{j}^{2}(t)}U\left(\frac{x-\xi_{j}(t)}{\lambda_{j}(t)}\right)(1+o(1)), U(y)=\frac{8}{(1+|y|^{2})^{2}},$$ with $\lambda_{j}(t) \approx 2e^{-\frac{\gamma+2}{2}}\sqrt{T-t}e^{-\sqrt{\frac{|\ln(T-t)|}{2}}} $ where $\gamma=0.57721...$ is the Euler-Mascheroni constant, $\xi_{j}(t)\to q_{j}\in \mathbb{R}^{2}$ and such that $\int_{\mathbb{R}^2}u(x,t)dx=km.$ This construction generalizes the existence result of the stable blow-up dynamics recently proved in \cite{CGMN1,CGMN2}.

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Cited by 2 Pith papers

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  1. Nonradial stability of self-similar blowup to Keller-Segel equation in three dimensions

    math.AP 2025-01 conditional novelty 8.0 of 10

    Any sufficiently small H^2 nonradial perturbation of the explicit 3D Keller-Segel self-similar blowup profile still blows up along the same self-similar profile with decaying error.

  2. Finite-time blow-up for the three dimensional axially symmetric Keller-Segel system

    math.AP 2025-08 conditional novelty 6.0 of 10

    For any finite set of points in the half-plane of axial symmetry, there exists a 3D Keller-Segel solution whose mass concentrates at those points with a precisely quantified finite-time blow-up rate.

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