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23 April 2024
 
  » arxiv » gr-qc/0404112

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The inverse mean curvature flow in Robertson-Walker spaces and its application to cosmology
Claus Gerhardt ;
Date 27 Apr 2004
Subject General Relativity and Quantum Cosmology; Differential Geometry | gr-qc hep-th math.DG
AbstractWe consider the inverse mean curvature flow in Robertson-Walker spacetimes that satisfy the Einstein equations and have a big crunch singularity and prove that under natural conditions the rescaled inverse mean curvature flow provides a smooth transition from big crunch to big bang. We also construct an example showing that in general the transition flow is only of class $C^3$.
Source arXiv, gr-qc/0404112
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