Accelerating Universe with a dynamic cosmological term

dc.creatorRay, Saibal
dc.creatorMukhopadhyay, Utpal
dc.creatorMeng, Xin-He
dc.date2004-07-14
dc.date2007-06-04
dc.date.accessioned2026-07-07T11:08:19Z
dc.date.available2026-07-07T11:08:19Z
dc.descriptionKeeping in mind the current picture of an accelerating and flat Universe, some specific dynamical models of the cosmological term $Λ$ have been selected for investigating the nature of dark energy. Connecting the free parameters of the models with the cosmic matter and vacuum energy density parameters, it is shown that the models are equivalent. Using the selected models, the present values of some of the physical parameters have been estimated, and a glimpse at the past decelerating universe has also been presented. It is observed that most of these cosmological parameters nicely agree with the values suggested by the Type Ia Supernovae and other experimental data.
dc.description9 Latex pages with considerable changes tthroughout the article with addition of an appendix and more references
dc.identifierhttps://arxiv.org/abs/astro-ph/0407295
dc.identifierhttp://arxiv.org/abs/astro-ph/0407295
dc.identifierGrav.Cosmol.13:142-150,2007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190096
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAccelerating Universe with a dynamic cosmological term
dc.typetext

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