The initial conditions of the Universe and holography

Details The initial conditions of the Universe and holography The initial conditions of the Universe and holography

2005-12-07

arxiv.org/abs/gr-qc/0512045v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Talk presented at the XXVIII Spanish Relativity Meeting E.R.E. 2005, Oviedo, September 6-10, 2005, to be published by AIP Conf

Scientific paper

10.1063/1.2218248

We address the initial conditions for an expanding cosmology using the holographic principle. For the case of a closed model, the old prescription of Fishler and Susskind, that uses the particle horizon to encode the bulk degrees of freedom, can be implemented for accelerated models with enough acceleration. As a bonus we have singularity free bouncing models. The bound is saturated for co-dimension one branes dominated universes.

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