Brane Universe and Standard Cosmology

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dc.creatorGong, Yungui
dc.date2000-05-17
dc.date.accessioned2026-07-07T03:24:57Z
dc.date.available2026-07-07T03:24:57Z
dc.descriptionBrane cosmology takes the unconventional form $H\sim \sqrtρ$. To recover the standard cosmology, we have to assume that the matter density is much less than the brane tension. We show that the assumption can be justified even near the end of inflation if we fine-tune the coupling constant of the inflaton potential. As a consequence, the standard cosmology is recovered after inflation.
dc.description5 pages, no figure
dc.identifierhttps://arxiv.org/abs/gr-qc/0005075
dc.identifierhttp://arxiv.org/abs/gr-qc/0005075
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33541
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleBrane Universe and Standard Cosmology
dc.typetext

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