Abstract
We consider the parabolic–elliptic Keller–Segel system *ut=Δu-χ∇·(u∇v),0=Δv-v+u\\documentclass[12pt]{minimal} \\usepackage{amsmath} \\usepackage{wasysym} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{amsbsy} \\usepackage{mathrsfs} \\usepackage{upgreek} \\setlength{\\oddsidemargin}{-69pt} \\begin{document}$$\\begin{aligned} \\left\\{ \\begin{aligned} u_t&= \\Delta u - \\chi \ abla \\cdot (u \ abla v), \\\\ 0&= \\Delta v - v + u \\end{aligned} \\right. \\end{aligned}$$\\end{document}in a smooth bounded domain Omega subseteq {mathbb {R}}^n, nin {mathbb {N}}, with Neumann boundary conditions. We look at both chemotactic attraction (chi > 0) and repulsion (chi < 0) scenarios in two and three dimensions. The key feature of interest for the purposes of this paper is under which conditions said system still admits global classical solutions due to the smoothing properties of the Laplacian even if the initial data is very irregular. Regarding this, we show for initial data mu in {mathcal {M}}_+({overline{Omega }}) that, if eithern = 2, chi < 0 orn = 2, chi > 0 and the initial mass is small orn = 3, chi < 0 and mu = f in L^p(Omega ), p > 1 holds, it is still possible to construct global classical solutions to (star ), which are continuous in t = 0 in the vague topology on {mathcal {M}}_+({overline{Omega }}).
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