2022
DOI: 10.3329/jsr.v14i3.56416
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Role of <i>f</i>(<i>R,T</i>) Gravity in Bianchi Type-V Dark Energy Model with Electromagnetic Field based on Lyra Geometry

Abstract: In this paper, a Bianchi type V Dark energy cosmological model scenario is studied with the electromagnetic field in Lyra based on  f(R,T) gravity. The source of the magnetic field is along the x axis. Field equations found in Lyra geometry with electromagnetic field  (F23 ≠ 0) in f(R,T) gravity, by choosing  f(R~,T) = f1(R~) + f2(T) with f1(R~) + μR~ and f2(T) = μT. A hybrid scale factor discusses the physical and dynamical aspects of f(R,T) gravity.

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Cited by 4 publications
(5 citation statements)
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“…Our aim is to derive the exact solutions of the field equations by assuming the following two extra conditions: i) The special law of variation for the Hubble parameter proposed by Berman [28], which yields a constant deceleration parameter defined by ̈ ̇ = Constant (25) ii) Assuming that the shear scalar is proportional to scalar expansion proposed by Collins [29], which leads to a condition (26) where is constant, and it takes care of the anisotropic nature of the model. Solving equation ( 25) yields to , (27) where and are constants of integration. This equation point towards the condition for the accelerated expansion of the universe is .…”
Section: Solution Of Field Equationsmentioning
confidence: 99%
See 1 more Smart Citation
“…Our aim is to derive the exact solutions of the field equations by assuming the following two extra conditions: i) The special law of variation for the Hubble parameter proposed by Berman [28], which yields a constant deceleration parameter defined by ̈ ̇ = Constant (25) ii) Assuming that the shear scalar is proportional to scalar expansion proposed by Collins [29], which leads to a condition (26) where is constant, and it takes care of the anisotropic nature of the model. Solving equation ( 25) yields to , (27) where and are constants of integration. This equation point towards the condition for the accelerated expansion of the universe is .…”
Section: Solution Of Field Equationsmentioning
confidence: 99%
“…Basumatary et al [26] have explored the Bianchi type VI 0 dark energy model with a particular form of scale factor in Sen-Dunn's theory of gravitation. Brahma et al [27] have reviewed Bianchi type-V dark energy cosmological model with the electromagnetic field in Lyra based on gravity. Inspired by the above discussions, in this paper, a higher dimensional bulk viscous fluid cosmological model with one-dimensional cosmic string is studied in the presence of interacting zero mass scalar field in Lyra geometry with the aid of Bianchi type-III spacetime.…”
Section: Introductionmentioning
confidence: 99%
“…Johri and Sudharsan have studied bulk viscous cosmological models in the Brans-Dicke theory of gravitation [30]. Several researchers [31][32][33][34][35][36][37] have recently explored the Bianchi type and Kaluza-Klein bulk viscous string cosmological models in the Saez-Ballester theory and the f (R, T) modified theory of gravity.…”
Section: Introductionmentioning
confidence: 99%
“…Brahma et al [61] have explored the Bianchi type V dark energy model with the electromagnetic field in Lyra based on ( ) theory of gravity. Ugale et al [62] studied the Bianchi type IX cosmological model with perfect fluid in ( ) theory of gravity.…”
Section: Introductionmentioning
confidence: 99%