2007
DOI: 10.1007/s10773-007-9617-6
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Kaluza-Klein Type Robertson Walker Cosmological Model with Dynamical Cosmological Term Λ

Abstract: In this paper we have analyzed the Kaluza-Klein type Robertson Walker (RW) cosmological models by considering three different forms of variable Λ: Λ ∼ ȧ a 2 , Λ ∼ ä 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 dimen… Show more

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Cited by 14 publications
(2 citation statements)
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“…The cosmological term is a variable that depends on the values of G, ρ, H 2 and Ḣ. These equations are related to H for a known value of Λ and many authors have been worked on this assumption [122,123] .…”
Section: Solution Of the Field Equationsmentioning
confidence: 99%
“…The cosmological term is a variable that depends on the values of G, ρ, H 2 and Ḣ. These equations are related to H for a known value of Λ and many authors have been worked on this assumption [122,123] .…”
Section: Solution Of the Field Equationsmentioning
confidence: 99%
“…Substituting G, ξ and in (20), it follows that, R R + 3γ (n + 3)(n + 1) − 6(n + 1) − αγ (n + 3) 6(n + 1)…”
Section: Case (Ii)mentioning
confidence: 99%