Cosmology and Modulus Stabilization in the Randall-Sundrum Setup with Bulk Matter

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dc.creatorKyae, Bumseok
dc.date2000-11-15
dc.date.accessioned2026-07-07T04:10:55Z
dc.date.available2026-07-07T04:10:55Z
dc.descriptionWe provide the exact time-dependent cosmological solutions in the Randall-Sundrum (RS) setup with bulk matter, which may be smoothly connected to the static RS metric. In the static limit of the extra dimension, the solutions are reduced to the standard Friedmann equations. In view of our solutions, we also propose an explanation for how the extra dimension is stabilized in spite of a flat modulus potential at the classical level.
dc.description10 pages, Proceeding of the talk at COSMO-2000, 4-th International Workshop on Particle physics and the Early Universe, at Cheju-Island, Korea, Sept. 4-8, 2000
dc.identifierhttps://arxiv.org/abs/hep-th/0011143
dc.identifierhttp://arxiv.org/abs/hep-th/0011143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50384
dc.subjectHigh Energy Physics - Theory
dc.titleCosmology and Modulus Stabilization in the Randall-Sundrum Setup with Bulk Matter
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