In this paper, we have studied Bianchi type-I string cosmological model by combining Kaluza-Klein (KK) theory and
theory of gravity which is an extension of 5-dimensional KK string cosmological models. We have used equation of state in the form of p-string or Takabayasi string given by
1
, where
ρ
and
λ
denote the rest density of energy cloud of strings, and the tension density of the system of strings, respectively and
ω
is a constant. In order to get physically significant and viable solution various forms of the function
are assumed, in this paper we assume
(e.g. Astashenok et al. (2017)
[1]
), where
α
is real number. Some physical and geometrical properties of the model are also discussed.
An exact solution of the vacuum Einstein field equations (VE-FEs) has been obtained of a spatially homogeneous and anisotropic (SHA) Bianchi type-I cosmological model by Kasner. The Kasner metric is shown to be a special case, and the exact vacuum solution of Kasner form model is obtained. Some physical properties of the model have been discussed.
In this paper, we attempt to study spatially homogeneous Bianchi types-III, V, VI 0 & VI h cosmological models in f (R, T) theory of gravity. Here the models are obtained by assuming forms of the function f (R, T) as f (R, T) = R + 2 f (T) and f (R, T) = f 1 (R) + f 2 (T). The exact solutions of Einstein's field equations (EFEs) have been obtained for two different types of physically viable cosmologies using a special form of Hubble parameter (HP). The physical and geometrical properties of these models have been discussed and expressions for the Ricci scalar R in each case are obtained.
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