On brane cosmological solutions

dc.creatorJassal, H. K.
dc.date2002-03-25
dc.date.accessioned2026-07-07T04:13:18Z
dc.date.available2026-07-07T04:13:18Z
dc.descriptionThis paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundrum brane scenario. The radius of the compact extra dimension is taken to be time dependent. It is shown that the cosmology consistent with the two brane Randall-Sundrum model is a power law expansion of the universe, with scale factor growing as $t^{1/2}$. The two branes tend to move towards each other with time. Some comments are made on the contribution of surface terms in deriving the four dimensional effective action.
dc.description8 pages, Latex2e
dc.identifierhttps://arxiv.org/abs/hep-th/0203224
dc.identifierhttp://arxiv.org/abs/hep-th/0203224
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51210
dc.subjectHigh Energy Physics - Theory
dc.titleOn brane cosmological solutions
dc.typetext

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