New infrared cut-off for the holographic scalar fields models of dark energy

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dc.creatorGranda, L. N.
dc.creatorOliveros, A.
dc.date2008-10-20
dc.date2008-10-23
dc.date.accessioned2026-07-07T12:37:29Z
dc.date.available2026-07-07T12:37:29Z
dc.descriptionIntroducing a new infrared cut-off for the holographic dark-energy, we study the correspondence between the quintessence, tachyon, K-essence and dilaton energy density with this holographic dark energy density in the flat FRW universe. This correspondence allows to reconstruct the potentials and the dynamics for the scalar fields models, which describe accelerated expansion.
dc.description12 pages, references added
dc.identifierhttps://arxiv.org/abs/0810.3663
dc.identifierhttp://arxiv.org/abs/0810.3663
dc.identifierPhys.Lett.B671:199-202,2009
dc.identifierdoi:10.1016/j.physletb.2008.12.025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218457
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNew infrared cut-off for the holographic scalar fields models of dark energy
dc.typetext

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