Generalized Model for $Λ$-Dark Energy

dc.creatorMukhopadhyay, Utpal
dc.creatorRay, P. C.
dc.creatorRay, Saibal
dc.creatorChoudhury, S. B. Datta
dc.date2008-02-07
dc.date.accessioned2026-07-07T13:13:16Z
dc.date.available2026-07-07T13:13:16Z
dc.descriptionEinstein field equations under spherically symmetric space-times are considered here in connection to dark energy investigation. A set of solutions are obtained for a kinematical $Λ$ model, viz., $Λ\sim (\dot a/a)^2$ without assuming any {\it a priori} value for the curvature constant and the equation of state parameter $ω$. Some interesting results, such as the nature of cosmic density $Ω$ and deceleration parameter $q$, have been obtained with the consideration of two-fluid structure instead of usual uni-fluid cosmological model.
dc.description8 Latex pages
dc.identifierhttps://arxiv.org/abs/0802.1032
dc.identifierhttp://arxiv.org/abs/0802.1032
dc.identifierInt.J.Mod.Phys.D18:389-396,2009
dc.identifierdoi:10.1142/S021827180901456X
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229834
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGeneralized Model for $Λ$-Dark Energy
dc.typetext

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