Holographic Dark Energy Model with Modified Generalized Chaplygin Gas

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dc.creatorPaul, B. C.
dc.creatorThakur, P.
dc.creatorSaha, A.
dc.date2007-07-31
dc.date2007-11-21
dc.date.accessioned2026-07-07T08:43:52Z
dc.date.available2026-07-07T08:43:52Z
dc.descriptionWe present a holographic dark energy model of the universe considering modified generalized Chaplygin gas (GCG). The modified GCG behaves as an ordinary barotropic fluid in the early epoch when the universe was tiny but behaves subsequently as a $Λ$CDM model at late epoch. An equivalent model with scalar field is obtained here by constructing the corresponding potential. The holographic dark energy is identified with the modified GCG and we determine the corresponding holographic dark energy field and its potential. The stability of the holographic dark energy in this case is also discussed.
dc.description15 Pages, 1 figure
dc.identifierhttps://arxiv.org/abs/0707.4625
dc.identifierhttp://arxiv.org/abs/0707.4625
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142464
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHolographic Dark Energy Model with Modified Generalized Chaplygin Gas
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