Extended Holographic dark energy

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dc.creatorGong, Yungui
dc.date2004-04-04
dc.date2004-09-16
dc.date.accessioned2026-07-07T11:32:16Z
dc.date.available2026-07-07T11:32:16Z
dc.descriptionThe idea of relating the infrared and ultraviolet cutoffs is applied to Brans-Dicke theory of gravitation. We find that extended holographic dark energy from the Hubble scale or the particle horizon as the infrared cutoff will not give accelerating expansion. The dynamical cosmological constant with the event horizon as the infrared cutoff is a viable dark energy model.
dc.descriptionone reference is corrected, 3 pages, no figure,V3: minor corrections
dc.identifierhttps://arxiv.org/abs/hep-th/0404030
dc.identifierhttp://arxiv.org/abs/hep-th/0404030
dc.identifierPhys.Rev.D70:064029,2004
dc.identifierdoi:10.1103/PhysRevD.70.064029
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/197538
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExtended Holographic dark energy
dc.typetext

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