Blowup for the Euler and Euler-Poisson Equations with Repulsive Forces

preprint2010arXivOpen access

Abstract

In this paper, we study the blowup of the NN-dim Euler or Euler-Poisson equations with repulsive forces, in radial symmetry. We provide a novel integration method to show that the non-trivial classical solutions (ρ,V)(ρ,V), with compact support in [0,R][0,R], where R>0R>0 is a positive constant and in the sense which ρ(t,r)=0ρ(t,r)=0 and V(t,r)=0V(t,r)=0 for r≥Rr\geq R, under the initial condition% H0=∫0RrV0dr>0H_{0}=\int_{0}^{R}rV_{0}dr>0 blow up on or before the finite time T=R3/(2H0)T=R^{3}/(2H_{0}) for pressureless fluids or γ>1.γ>1. The main contribution of this article provides the blowup results of the Euler (δ=0)(δ=0) or Euler-Poisson (δ=1)(δ=1) equations with repulsive forces, and with pressure (γ>1)(γ>1), as the previous blowup papers (\cite{MUK} \cite{MP}, \cite{P} and \cite{CT}) cannot handle the systems with the pressure term, for C1C^{1} solutions.

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