Corners and collapse: Some simple observations concerning critical masses and boundary blow-up in the fully parabolic Keller-Segel system
arXiv:2305.18839 · doi:10.1016/j.aml.2023.108788
Abstract
Our main result shows that the mass is critical for the minimal Keller-Segel system \begin{align}\label{prob:abstract}\tag{} \begin{cases} u_t = Δu - \nabla \cdot (u \nabla v), \\ v_t = Δv - v + u, \end{cases} \end{align} considered in a quarter disc , , in the following sense: For all reasonably smooth nonnegative initial data with , there exists a global classical solution to the Neumann initial boundary value problem associated to \eqref{prob:abstract}, while for all there exist nonnegative initial data with so that the corresponding classical solution of this problem blows up in finite time. At the same time, this gives an example of boundary blow-up in \eqref{prob:abstract}. Up to now, precise values of critical masses had been observed in spaces of radially symmetric functions or for parabolic-elliptic simplifications of \eqref{prob:abstract} only.
7 pages