Holographic Principle during Inflation and a Lower Bound on Density Fluctuations

Preprint

4 December 1998

preprint
Published by arXiv in arXiv

Abstract

We apply the holographic principle during the inflationary stage of our universe. Where necessary, we illustrate the analysis in the case of new and extended inflation which, together, typify generic models of inflation. We find that in the models of extended inflation type, and perhaps of new inflation type also, the holographic principle leads to a lower bound on the density fluctuations.

Keywords

PRINCIPLE DURING INFLATION
HOLOGRAPHIC PRINCIPLE
DENSITY FLUCTUATIONS
EXTENDED INFLATION
PRINCIPLE LEADS
INFLATION TYPE
LOWER BOUND

All Related Versions

Version 1, 1998-12-04, ArXiv
Version 2, 1998-12-19, ArXiv
Published version: Physics Letters B, 450 (1-3), 55.

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