Holographic temperature bound in the slow-roll inflation

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dc.creatorMyung, Y. S.
dc.date2003-07-04
dc.date.accessioned2026-07-07T04:15:25Z
dc.date.available2026-07-07T04:15:25Z
dc.descriptionWe 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.
dc.description9 pages, 1figure
dc.identifierhttps://arxiv.org/abs/hep-th/0307045
dc.identifierhttp://arxiv.org/abs/hep-th/0307045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51991
dc.subjectHigh Energy Physics - Theory
dc.titleHolographic temperature bound in the slow-roll inflation
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