Inflation as a response to protect the Holographic Principle
arXiv:0908.0287 · doi:10.1142/S0217732309030758
Abstract
A model where the inflationary phase emerges as a response to protect the Fischler-Susskind holographic bound is described. A two fluid model in a closed universe inflation picture is assumed, and a discussion on conditions under which is possible to obtain an additional exponential expansion phase as those currently observed is given.
6 pages, 2 figures. Accepted for publication in MPLA
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