Anisotropic Bianchi type-III perfect fluid cosmological models in f(R, T) theory of gravity

Chandel, S.; Ram, Shri

doi:10.1007/s12648-013-0362-9

Cited by 37 publications

(12 citation statements)

References 24 publications

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“…Now, solving Eq. ( 12) we obtain three different solutions given as (13) where a 0 , a 1 , a 2 , c 1 , c 2 , c 3 are constants of integration. It may be noted that the last two of the solutions in Eq.…”

Section: F (R T) Gravity Field Equations and Kk Modelsmentioning

confidence: 99%

“…Many authors have investigated perfect fluid cosmological models in this particular theory. Adhav [12] discussed Bianchi type-I perfect fluid model in f (R, T) gravity while Chandel and Shri Ram [13] and Reddy et al [14] have investigated several aspects of Bianchi type-III perfect fluid cosmological models in this theory. Sharif and Zubair [15] have obtained anisotropic universe models with perfect fluid and scalar field in this particular theory of gravity.…”

Section: Introductionmentioning

confidence: 99%

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Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity

Reddy¹,

Aditya²

2018

Int J Phys Stud Res

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Here, we investigate cosmological models with perfect fluid source in the framework of Kaluza-Klein FRW space time in a modified theory of gravity known as f (R, T) gravity (Harko et al. 2011) where R is the Ricci scalar and T is the trace of the stress energy tensor of the perfect fluid. By solving the field equations, we have found an exact solution of the field equations using a linearly varying deceleration parameter which can be considered as a five dimensional FRW type cosmological model in f (R, T) gravity. We have determined the spatial volume and average Hubble parameter of the model. We have also determined and discussed the physical parameters, pressure and density for dust, radiation and stiff matter dominated eras.

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Section: F (R T) Gravity Field Equations and Kk Modelsmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity

Reddy¹,

Aditya²

2018

Int J Phys Stud Res

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“…Katore et al [8] investigated some cosmological model with DE source in ) , ( T R f gravity. Chandel and Ram [9] generated new classes of solutions of field equations starting from known solutions for an anisotropic Bianchi type-III cosmological model with perfect fluid in ) , ( T R f gravity. Chaubey et al [10] has obtained a new class of Bianchi type cosmological models in ) , ( T R f gravity, while, Sahoo et al [11] investigated an axially symmetric space-time in the presence of a perfect fluid source within the frame work of ) , ( T R f gravity.…”

Section: Introductionmentioning

confidence: 99%

Accelerating Universe with Viscous Cosmic String in Quadratic Form of Teleparallel Gravity

Bhoyar¹,

Chirde²,

Shekh³

2019

J. Sci. Res.

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In this paper, we have investigated Kantowaski-Sachs cosmological model with bulk viscous and cosmic string in the framework of Teleparallel Gravity so called f(T) gravity, where T denotes the torsion scalar. The behavior of accelerating universe is discussed towards the particular choice of f(T) = Α(T) + β(T)m. The exact solutions of the field equations are obtained by applying variable deceleration parameter which is linear in time with a negative slope. The physical behavior of these models has been discussed using some physical quantities. Also, the function of the torsion scalar for the universe is evaluated.

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“…This provides a strong motivation to look for some alternative models to explain such anisotropy. Bianchi models [39][40][41][42][43][44][45][46][47][48][49][50][51][52][53] pave a way for the researchers to describe the anisotropic phase of early universe and the acceleration phase of late universe.…”

Section: Introductionmentioning

confidence: 99%

Bianchi I and V cosmologies with Hu-Sawicki f(R) gravity in Palatini formalism

Banik

Bhuyan

2018

J. Phys. Commun.

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The main objective of this work is the pursuit of a detailed analysis of the cosmological solutions corresponding to each fixed point belonging to an exclusive form of f (R) initially introduced by Hu and Sawicki in the background of Palatini f (R) gravity. Fixed points and their associated solutions for the anisotropic Bianchi type I and V models are derived by utilizing an approach used to solve autonomous ordinary differential equations. Building on this background, an exhaustive study on the phase space is accomplished and the existence of a sequence of evolution that starts from unstable anisotropic universe to a stable phase of late times de Sitter expansion through the standard radiation and matter dominated era has been established.

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Anisotropic Bianchi type-III perfect fluid cosmological models in f(R, T) theory of gravity

Cited by 37 publications

References 24 publications

Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity

Kaluza-Klein FRW type Perfect Fluid Cosmological Models with Linearly varying Deceleration Parameter in a Modified Gravity

Accelerating Universe with Viscous Cosmic String in Quadratic Form of Teleparallel Gravity

Bianchi I and V cosmologies with Hu-Sawicki f(R) gravity in Palatini formalism

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