Abstract
We prove that, for a given spherically symmetric fluid distribution with tangential pressure on an initial space-like hypersurface with a time-like boundary, there exists a unique, local in time solution to the Einstein equations in a neighbourhood of the boundary. As an application, we consider a particular elastic fluid interior matched to a vacuum exterior.
Funder
CMAT, Univ. Minho, through FEDER
Subject
General Physics and Astronomy,General Engineering,General Mathematics
Cited by
2 articles.
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1. Rigid elastic solids in relativity;Classical and Quantum Gravity;2020-10-30
2. Elastic shocks in relativistic rigid rods and balls;Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences;2019-05