Issue |
EAS Publications Series
Volume 30, 2008
Spanish Relativity Meeting - Encuentros Relativistas Españoles , ERE2007: Relativistic Astrophysics and Cosmology
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Page(s) | 367 - 371 | |
DOI | https://doi.org/10.1051/eas:0830063 | |
Published online | 30 September 2008 |
A. Oscoz, E. Mediavilla and M. Serra-Ricart (eds)
EAS Publications Series, 30 (2008) 367-371
Saturation of the Holographic Principle for Spatially Closed Cosmological Models
Deptartamento de Fisica Teorica, Facultad de Ciencias, Universidad de Zaragoza,
Spain
Corresponding authors: pablo@posta.unizar.es ; maperb@gmail.com ; segui@posta.unizar.es
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.
© EAS, EDP Sciences, 2008