Holographic Cosmological Models on the Braneworld

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dc.creatorLepe, Samuel
dc.creatorPena, Francisco
dc.creatorSaavedra, Joel
dc.date2008-06-05
dc.date.accessioned2026-07-07T12:36:01Z
dc.date.available2026-07-07T12:36:01Z
dc.descriptionIn this article we have studied a closed universe which a holographic energy on the brane whose energy density is described by $ρ(H) =3c^{2}H^{2}$ and we obtain an equation for the Hubble parameter, this equation gave us different physical behavior depending if $c^2>1$ or $c^2<1$ against of the sign of the brane tension.
dc.identifierhttps://arxiv.org/abs/0806.0981
dc.identifierhttp://arxiv.org/abs/0806.0981
dc.identifierPhys.Lett.B671:323-326,2009
dc.identifierdoi:10.1016/j.physletb.2008.12.048
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217955
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHolographic Cosmological Models on the Braneworld
dc.typetext

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