Continued Gravitational Collapse for Newtonian Stars

2018/11/05 by Guo, Yan, Hadzic, Mahir, Jang, Juhi
#35B44 #35L81 #35Q31 #35Q75 #76N15 #Analysis of PDEs (math.AP) #FOS: Mathematics #FOS: Physical sciences #Mathematical Physics (math-ph)

paper · doi:10.48550/arxiv.1811.01616

Abstract

The classical model of an isolated selfrgavitating gaseous star is given by the Euler-Poisson system with a polytropic pressure law P(ρ)=ρ^γ, γ>1. For any 1

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