Kaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term Lambda

dc.contributor.authorPradhan, Anirudh
dc.contributor.authorKhadekar, G. S.
dc.contributor.authorPatki, Vrishali
dc.date.accessioned2012-03-06T07:13:22Z
dc.date.available2012-03-06T07:13:22Z
dc.date.issued2005-12-01
dc.description.abstractIn this paper we have analyzed the Kaluza-Klein type RobertsonWalker (RW) cosmological models by considering three different forms of variable Λ: Λ ∼˙ a a 2 , Λ ∼ ¨ a a and Λ ∼ ρ. It is found that, the connecting free parameters of the models with cosmic matter and vacuum energy density parameters are equivalent, in the context of higher dimensional space time. The expression for the look back time, luminosity distance and angular diameter distance are also derived. This work has thus generalized to higher dimensions the well-known results in four dimensional space time. It is found that there may be significant difference in principle at least, from the analogous situation in four dimensional space time.en_US
dc.identifier.urihttp://hdl.handle.net/11007/662
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;36/05
dc.subjectHigher dimensional space timeen_US
dc.subjectCosmologyen_US
dc.subjectCosmological parametersen_US
dc.subjectCosmological testsen_US
dc.titleKaluza-Klein Type Robertson Walker Cosmological Model With Dynamical Cosmological Term Lambdaen_US
dc.typeArticleen_US

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