Can diffusion degeneracies enhance complexity in chemotactic aggregation? Finite-time blow-up on spheres in a quasilinear Keller–Segel system

The Cauchy problem in \mathbb{R}^{n} for the cross-diffusion system \begin{cases}u_{t} = \nabla \cdot (D(u)\nabla u) - \nabla\cdot (u\nabla v), \\ 0 = \Delta v +u,\end{cases} is considered for n\ge 2 and under assumptions ensuring that D suitably generalizes the prototype given by D(\xi)=(\xi+1)^{-\alpha}, \quad \xi\ge 0. Under the assumption that \alpha>1 , it is shown that for any r_{\star}>0 and \delta\in (0,1) one can find radially symmetric initial data from C_{0}^{\infty}(\mathbb{R}^{n}) such that the corresponding solution blows up within some finite time, and that this explosion occurs throughout certain spheres in an appropriate sense, with any such sphere being located in the annulus \overline{B}_{r_\star+\delta}(0)\setminus B_{(1-\delta)r_\star}(0) .This is complemented by a result revealing that when \alpha<1 , any finite-mass unbounded radial solution must blow up exclusively at the spatial origin.

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Publication Details

Journal
Journal of the European Mathematical Society
Published
2025-02-13
DOI
https://doi.org/10.4171/jems/1607
Citations
1
Primary Topic
Mathematical Biology Tumor Growth
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article
Field-Weighted Citation Impact
1.37
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article

Can diffusion degeneracies enhance complexity in chemotactic aggregation? Finite-time blow-up on spheres in a quasilinear Keller–Segel system

Michael Winkler
1 citations
Journal of the European Mathematical Society
Mathematical Biology Tumor Growth
1.37
article

Can diffusion degeneracies enhance complexity in chemotactic aggregation? Finite-time blow-up on spheres in a quasilinear Keller–Segel system

Michael Winkler
article en
1 citations

Abstract

The Cauchy problem in \mathbb{R}^{n} for the cross-diffusion system \begin{cases}u_{t} = \nabla \cdot (D(u)\nabla u) - \nabla\cdot (u\nabla v), \\ 0 = \Delta v +u,\end{cases} is considered for n\ge 2 and under assumptions ensuring that D suitably generalizes the prototype given by D(\xi)=(\xi+1)^{-\alpha}, \quad \xi\ge 0. Under the assumption that \alpha>1 , it is shown that for any r_{\star}>0 and \delta\in (0,1) one can find radially symmetric initial data from C_{0}^{\infty}(\mathbb{R}^{n}) such that the corresponding solution blows up within some finite time, and that this explosion occurs throughout certain spheres in an appropriate sense, with any such sphere being located in the annulus \overline{B}_{r_\star+\delta}(0)\setminus B_{(1-\delta)r_\star}(0) .This is complemented by a result revealing that when \alpha<1 , any finite-mass unbounded radial solution must blow up exclusively at the spatial origin.

Journal of the European Mathematical Society
Paderborn University (DE)
Openalex Percentile: Top 26%
Mathematical Biology Tumor Growth
1.37
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