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On future geodesic completeness for the Einstein-Vlasov system with hyperbolic symmetry

2002/03/20 by Gerhard Rein
Physics and Astronomy · #gr-qc

paper · pdf · doi:10.1017/s0305004103007485

published as Math.Proc.Cambridge Phil.Soc. 137 (2004) 237-244 · 8 pages

arxiv created 2002/03/20 · arxiv updated 2009/11/30

Abstract

Spacetimes with collisionless matter evolving from data on a compact Cauchy surface with hyperbolic symmetry are shown to be timelike and null geodesically complete in the expanding direction, provided the data satisfy a certain size restriction.

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