Closed universes can satisfy the holographic principle in three dimensions
arXiv:hep-th/0110175 · doi:10.1016/S0370-2693(01)01234-5
Abstract
We examine in details Friedmann-Robertson-Walker models in 2+1 dimensions in order to investigate the cosmic holographic principle suggested by Fischler and Susskind. Our results are rigorously derived differing from the previous one found by Wang and Abdalla. We discuss the erroneous assumptions done in this work. The matter content of the models is composed of a perfect fluid, with a -law equation of state. We found that closed universes satisfy the holographic principle only for exotic matter with a negative pressure. We also analyze the case of a collapsing flat universe.
14 pages, latex, no figures.Accepted in Phys.Lett.B
References in corpus (6)
- A Covariant Entropy Conjecture
- Proof of Classical Versions of the Bousso Entropy Bound and of the Generalized Second Law
- Cosmology vs. Holography
- TASI lectures on the Holographic Principle
- Cosmological scaling solutions of minimally coupled scalar fields in three dimensions
- Holography in (2+1)-dimensional cosmological models