Bianchi Type-I Universe in Modified Theory of Gravity
In this paper, we have studied an anisotropic Bianchi-I cosmological model in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>R</mi><mo>,&l...
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MDPI AG
2023-02-01
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author | Bhupendra Kumar Shukla Rishi Kumar Tiwari Aroonkumar Beesham |
author_facet | Bhupendra Kumar Shukla Rishi Kumar Tiwari Aroonkumar Beesham |
author_sort | Bhupendra Kumar Shukla |
collection | DOAJ |
description | In this paper, we have studied an anisotropic Bianchi-I cosmological model in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>R</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity. To obtain the exact solutions of the field equations, we have used the condition <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>σ</mi><mo>/</mo><mi>θ</mi></mrow></semantics></math></inline-formula> to be a function of the scale factor (<b>IJTP, 54, 2740-2757, 2015</b>). Our model possesses an initial singularity. It initially exhibits decelerating expansion and transits to accelerating expansion at late times. We have also discussed the physical and geometrical properties of the model. |
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spelling | doaj.art-b487b74d3be44615b6568919ef44b30e2023-11-18T12:20:31ZengMDPI AGPhysical Sciences Forum2673-99842023-02-01712810.3390/ECU2023-14049Bianchi Type-I Universe in Modified Theory of GravityBhupendra Kumar Shukla0Rishi Kumar Tiwari1Aroonkumar Beesham2Department of Mathematics, Government College, Bandri Sagar 470442, IndiaDepartment of Mathematics, Government Model Science College, Rewa 486001, IndiaFaculty of Natural Sciences, Mangosuthu University of Technology, Umlazi 4031, South AfricaIn this paper, we have studied an anisotropic Bianchi-I cosmological model in <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>f</mi><mo>(</mo><mi>R</mi><mo>,</mo><mi>T</mi><mo>)</mo></mrow></semantics></math></inline-formula> gravity. To obtain the exact solutions of the field equations, we have used the condition <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>σ</mi><mo>/</mo><mi>θ</mi></mrow></semantics></math></inline-formula> to be a function of the scale factor (<b>IJTP, 54, 2740-2757, 2015</b>). Our model possesses an initial singularity. It initially exhibits decelerating expansion and transits to accelerating expansion at late times. We have also discussed the physical and geometrical properties of the model.https://www.mdpi.com/2673-9984/7/1/28Bianchi Type-Ivariable anisotropy parameterequation of state parameter |
spellingShingle | Bhupendra Kumar Shukla Rishi Kumar Tiwari Aroonkumar Beesham Bianchi Type-I Universe in Modified Theory of Gravity Physical Sciences Forum Bianchi Type-I variable anisotropy parameter equation of state parameter |
title | Bianchi Type-I Universe in Modified Theory of Gravity |
title_full | Bianchi Type-I Universe in Modified Theory of Gravity |
title_fullStr | Bianchi Type-I Universe in Modified Theory of Gravity |
title_full_unstemmed | Bianchi Type-I Universe in Modified Theory of Gravity |
title_short | Bianchi Type-I Universe in Modified Theory of Gravity |
title_sort | bianchi type i universe in modified theory of gravity |
topic | Bianchi Type-I variable anisotropy parameter equation of state parameter |
url | https://www.mdpi.com/2673-9984/7/1/28 |
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