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Saturation of the Holographic Principle for Spatially Closed Cosmological Models

Published online by Cambridge University Press:  30 September 2008

A. Oscoz ,
E. Mediavilla ,
M. Serra-Ricart ,
P. Diaz ,
M.A. Per  and
A. Segui
P. Diaz*
Affiliation:
Deptartamento de Fisica Teorica, Facultad de Ciencias, Universidad de Zaragoza, Spain
M.A. Per
Affiliation:
Deptartamento de Fisica Teorica, Facultad de Ciencias, Universidad de Zaragoza, Spain
A. Segui
Affiliation:
Deptartamento de Fisica Teorica, Facultad de Ciencias, Universidad de Zaragoza, Spain
*
pablo@posta.unizar.es ; maperb@gmail.com ; segui@posta.unizar.es
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Abstract

Under the assumption on the fundamental character of the Holographic Principle as a primary principle guiding the behavior of our universe the saturation of the holographic limit is reasonable. On the other hand the Fischler-Susskind holographic prescription seems to be incompatible with closed cosmological models due to the apparently unavoidable recontraction of the particle horizon area. However we will show that the saturation of the Fischler-Susskind holographic prescription over a closed (although almost flat) cosmological model enforces a cosmological evolution very similar to the observed universe.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 30: Spanish Relativity Meeting - Encuentros Relativistas Españoles , ERE2007: Relativistic Astrophysics and Cosmology , 2008 , pp. 367 - 371
Copyright
© EAS, EDP Sciences, 2008

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References

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