Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario

Abstract The paper deals with cosmological solutions describing different phases of the Universe for the homogeneous and isotropic FLRW model of the Universe with torsion. Normally, torsion field is not suitable for maximally symmetric space time model. However, one may use a specific profile of vec...

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Main Authors: Akash Bose, Subenoy Chakraborty
Format: Article
Language:English
Published: SpringerOpen 2020-03-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-7771-7
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author Akash Bose
Subenoy Chakraborty
author_facet Akash Bose
Subenoy Chakraborty
author_sort Akash Bose
collection DOAJ
description Abstract The paper deals with cosmological solutions describing different phases of the Universe for the homogeneous and isotropic FLRW model of the Universe with torsion. Normally, torsion field is not suitable for maximally symmetric space time model. However, one may use a specific profile of vectorial torsion field, derived from a scalar function. By proper choices of the torsion scalar function, it is shown that a continuous cosmic evolution starting from the emergent scenario to the present late time acceleration is possible. Also thermodynamics of the system is analyzed and equivalence with Einstein gravity is discussed.
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spelling doaj.art-7ef4cb40bcfd4f49b043b2c4386884182022-12-22T01:06:39ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-03-018031810.1140/epjc/s10052-020-7771-7Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenarioAkash Bose0Subenoy Chakraborty1Department of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityAbstract The paper deals with cosmological solutions describing different phases of the Universe for the homogeneous and isotropic FLRW model of the Universe with torsion. Normally, torsion field is not suitable for maximally symmetric space time model. However, one may use a specific profile of vectorial torsion field, derived from a scalar function. By proper choices of the torsion scalar function, it is shown that a continuous cosmic evolution starting from the emergent scenario to the present late time acceleration is possible. Also thermodynamics of the system is analyzed and equivalence with Einstein gravity is discussed.http://link.springer.com/article/10.1140/epjc/s10052-020-7771-7
spellingShingle Akash Bose
Subenoy Chakraborty
Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
European Physical Journal C: Particles and Fields
title Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
title_full Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
title_fullStr Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
title_full_unstemmed Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
title_short Homogeneous and isotropic space-time, modified torsion field and complete cosmic scenario
title_sort homogeneous and isotropic space time modified torsion field and complete cosmic scenario
url http://link.springer.com/article/10.1140/epjc/s10052-020-7771-7
work_keys_str_mv AT akashbose homogeneousandisotropicspacetimemodifiedtorsionfieldandcompletecosmicscenario
AT subenoychakraborty homogeneousandisotropicspacetimemodifiedtorsionfieldandcompletecosmicscenario