Holographic temperature bound in the slow-roll inflation

2003/07/04 by Y. S. Myung, Myung, Y. S.
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Theory (hep-th) #hep-th

paper · pdf · doi:10.48550/arxiv.hep-th/0307045

9 pages, 1figure

arxiv created 2003/07/04 · arxiv updated 2009/11/30

Abstract

We investigate the relationship between the holographic temperature bound and the slow-roll inflation. For this purpose we introduce the holographic temperature bound for a radiation matter :T ≥ T_{\rm H}. Here T_{\rm H} is the Hubble temperature which arises from the cosmological holographic description of for a radiation-dominated universe. For the quasi-de Sitter phase of slow-roll inflation, we find that the holographic temperature bound of T_{\rm GH} ≥ T_{\rm H} is guaranteed with the Gibbons-Hawking temperature T_{\rm GH}. When T_{\rm GH}= T_{\rm H}, inflation ends.

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