Restoring Holographic Dark Energy in Brane Cosmology

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dc.creatorSaridakis, E. N.
dc.date2007-12-13
dc.date2008-01-17
dc.date.accessioned2026-07-07T11:13:44Z
dc.date.available2026-07-07T11:13:44Z
dc.descriptionWe present a generalized version of holographic dark energy arguing that it must be considered in the maximally subspace of a cosmological model. In the context of brane cosmology it leads to a bulk holographic dark energy which transfers its holographic nature to the effective 4D dark energy. As an application we use a single-brane model and we show that in the low energy limit the behavior of the effective holographic dark energy coincides with that predicted by conventional 4D calculations. However, a finite bulk can lead to radically different results.
dc.description11 pages, version published in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/0712.2228
dc.identifierhttp://arxiv.org/abs/0712.2228
dc.identifierPhys.Lett.B660:138-143,2008
dc.identifierdoi:10.1016/j.physletb.2008.01.004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191824
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleRestoring Holographic Dark Energy in Brane Cosmology
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