Interacting anisotropic dark energy with hybrid expansion in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si22.svg"><mml:mrow><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math> gravity

Singh, S. Surendra; Devi, L. Anjana

doi:10.1016/j.newast.2021.101656

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2022

2024

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Cited by 8 publications

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“…Recently, Bhardwaj et al [54] have explored dark energy models in f (R, T) gravity. Also, Singh and Devi [55] investigate the locally rotationally symmetric (LRS) Bianchi type-I cosmological models in gravity with Hybrid Expansion Law.…”

Section: Introductionmentioning

confidence: 99%

Role of f(R,T) Gravity in Bianchi Type-V Dark Energy Model with Electromagnetic Field based on Lyra Geometry

Brahma

Dewri

2022

J. Sci. Res.

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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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Section: Introductionmentioning

confidence: 99%