Holographic temperature bound in the slow-roll inflation

Details Holographic temperature bound in the slow-roll inflation Holographic temperature bound in the slow-roll inflation

2003-07-04

arxiv.org/abs/hep-th/0307045v1

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, 1figure

Scientific paper

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 :$T \ge T_{\rm H}$. 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 $T_{\rm GH} \ge T_{\rm H}$ is guaranteed with the Gibbons-Hawking temperature $T_{\rm GH}$. When $T_{\rm GH}= T_{\rm H}$, inflation ends.

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