Blow-up of solutions to the Keller-Segel model with tensorial flux in high dimensions

Over the course of the last decade, there has been a significant level of interest in the analysis of Keller-Segel models incorporating tensorial flux. Despite this interest, the question of whether finite-time blowup solutions exist remains a topic of ongoing research. Our study provides evidence that solutions of this nature are indeed possible in dimensions $n\ge 3,$ when utilizing a tensorial flux expressed in the form of $A\mathrm{\nabla }v$, where $A$ denotes a matrix with constant components