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arXiv · hep-th/0307258

Anatomy of a Bounce

A. J. M. Medved
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Abstract

Holographic considerations are used in the scrutiny of a special class of brane-world cosmologies. Inherently to this class, the brane typically bounces, at a finite size, as a consequence of a charged black hole in the bulk. Whereas a prior treatment [hep-th/0301010] emphasized a brane that is void of standard-model matter, the analysis is now extended to include an intrinsic (radiation-dominated) matter source. An interesting feature of this generalized model is that a bounce is no longer guaranteed but, rather, depends on the initial conditions. Ultimately, we demonstrate that compliance with an appropriate holographic bound is a sufficient prerequisite for a bounce to occur.

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A. J. M. Medved. 2004-03-25. Anatomy of a Bounce. https://doi.org/10.1088/0264-9381%2F21%2F11%2F016

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