[PDF] Top 20 Bianchi type-III Cosmological Model with Linear Equation of State in f(R) Gravity

... The prediction about expansion of the universe is flat, past decelerated and present accelerating can classified into two categories [1, 2]. One can measure due to mysterious energy with negative pressure dubbed as Dark ... See full document

... of f ( R , T ) ...symmetric cosmological models in f ( R , T ) theory of gravity with a term ...of gravity are considered by Shaikh ...of f ( R , T ) theory ... See full document

... in Bianchi type-V space time. Bianchi type models are among simplest models with anisotropy ...of Bianchi type–I and V space times in metric f (R ) gravity ... See full document

... multidimensional cosmological models in general relativity and in other alternative theories of ...dimensional cosmological model filled with perfect fluid in f(R,T) theory of ...of ... See full document

... paper, Bianchi type I space time in Kasner form with wet dark fluid (WDF), which is a candidate for dark energy (DE), in the framework of f(R, T) gravity, R and T denote the ... See full document

... of gravity in general relativity. 5-D Kaluza-Klein cosmological models with quark matter attached to the string cloud and domain walls have been studied by Yilmaz [60- 61] ...Kaluza-Klein ... See full document

... , gravity , where R is the Ricci scalar and T the trace of stress energy-momentum tensor in the context of late time accelerating expansion of the universe has been ...the cosmological model ... See full document

... Abstract Bianchi type III string cosmological models (massive and geometric) in presence of magnetic field with vacuum energy density following the techniques used by Letelier (1979) and ... See full document

... literature cosmological models with a constant deceleration parameter have been studied by Berman and Gomide (1988), Johri and Desikan (1994), Singh and Desikan (1997), Maharaj and Naidoo (1993), Pradhan et ...of ... See full document

... of Bianchi types-I (Kasner form) cosmological model in f(R) theory of gravity has been ...of Bianchi type-I space-time in Kasner form have been obtained with the ... See full document

... Modified theories of gravitation provide gravitational alternatives for dark energy to explain early inflation and late time acceleration of the universe. To extend the concept of theory of general relativity, Brans and ... See full document

... anisotropic cosmological universes with wet dark ...the Bianchi type- III and Kantowski-Sachs Universes with matter term with dark energy treated as a Dark Fluid satisfying the Equation ... See full document

... Cosmological constant is the energy density of the vacuum ...back gravity” and achieve a static ...vacuum state of all existing fields is the ...the cosmological constant in 1917.According to ... See full document

... fluid type by assuming an equation of state linking the pressure p and energy density in order to build an analytical methodsnear the ...variable equation of state, which essentially ... See full document

... of cosmological models with dark energy create much more interest due to the fact that our universe is undergoing an accelerated expansion which is driven by an exotic energy with large negative pressure named ... See full document

... universe. Cosmological model play a vital role in the understanding of the universe around ...consider cosmological model with dark ...(WDF) model was in the spirit of generalization ... See full document

... Motivated by above discussion, in this paper we have obtained exact solutions of the Einstein field equations of Bianchi type V Cosmological model with linear equation of state in the sc[r] ... See full document

... Equations (9)-(12) are four highly non-linear equations in six unknowns a , b ,  , p ,  and T . We can introduce more conditions either by an assumption corresponding to some physical situation or an arbitrary ... See full document

... with Bianchi type V cosmological model in the presence of perfect fluid with polytropic equation of state (EoS) p  K  n , where K and n are constants called as polytropic ... See full document

... candidates: cosmological constant, quintessence [4-6], k-essence [7-9], phantom energy ...Friedmann equation such as Cardassian expansion [13,14] as well as what might be derived from brane cosmology ... See full document