A Note on Holographic Principle in models of Extended Inflation type

Details A Note on Holographic Principle in models of Extended Inflation type A Note on Holographic Principle in models of Extended Inflation type

1999-08-08

arxiv.org/abs/hep-th/9908061v1

Physics

High Energy Physics

High Energy Physics - Theory

4 pages. Latex file

Scientific paper

We present a simple derivation of an upper bound on the average size of the true vacuum bubbles at the end of inflation, in models of extended inflation type. The derivation uses the inequality that the total energy inside a given volume must be less than its linear dimensions. The above bound is the same as that obtained earlier, by applying the holographic principle according to Fischler-Susskind prescription. Such a bound leads to a lower bound on the denisty fluctuations.

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