The initial conditions of the Universe and holography

Journal Article · Mon Jun 19 00:00:00 EDT 2006 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.2218248· OSTI ID:20873204

Diaz, Pablo; Per, Miguel Angel; Segui, Antonio ^[1]

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1. Departamento de Fisica Teorica, Universidad de Zaragoza. 50009-Zaragoza (Spain)

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.

• OSTI ID: 20873204
• Journal Information: AIP Conference Proceedings, Vol. 841, Issue 1; Conference: ERE 2005: 28. Spanish relativity meeting: A century of relativity physics, Oviedo, Asturias (Spain), 6-10 Sep 2006; Other Information: DOI: 10.1063/1.2218248; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ACCELERATION
COSMOLOGY
DEGREES OF FREEDOM
HOLOGRAPHY
MEMBRANES
QUANTUM FIELD THEORY
SINGULARITY
UNIVERSE