Holographic Dark Energy Scenario and Variable Modified Chaplygin Gas

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dc.creatorChattopadhyay, Surajit
dc.creatorDebnath, Ujjal
dc.date2009-01-15
dc.date.accessioned2026-07-07T12:51:30Z
dc.date.available2026-07-07T12:51:30Z
dc.descriptionIn this letter, we have considered that the universe is filled with normal matter and variable modified Chaplygin gas. Also we have considered the interaction between normal matter and variable modified Chaplygin gas in FRW universe. Then we have considered a correspondence between the holographic dark energy density and interacting variable modified Chaplygin gas energy density. Then we have reconstructed the potential of the scalar field which describes the variable modified Chaplygin cosmology.
dc.description4 latex pages, no figures, RevTeX style
dc.identifierhttps://arxiv.org/abs/0901.2184
dc.identifierhttp://arxiv.org/abs/0901.2184
dc.identifierAstrophys.Space Sci.319:183-185,2009
dc.identifierdoi:10.1007/s10509-009-9977-x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/223007
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHolographic Dark Energy Scenario and Variable Modified Chaplygin Gas
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