Universe consisting of diffusive dark fluids: thermodynamics and stability analysis

Abstract The present work deals with homogeneous and isotropic FLRW model of the Universe having a system of non-interacting diffusive cosmic fluids with barotropic equation of state (constant or variable equation of state parameter). Due to diffusive nature of the cosmic fluids, the divergence of t...

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Main Authors: Subhayan Maity, Pritikana Bhandari, Subenoy Chakraborty
Format: Article
Language:English
Published: SpringerOpen 2019-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-019-6603-0
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author Subhayan Maity
Pritikana Bhandari
Subenoy Chakraborty
author_facet Subhayan Maity
Pritikana Bhandari
Subenoy Chakraborty
author_sort Subhayan Maity
collection DOAJ
description Abstract The present work deals with homogeneous and isotropic FLRW model of the Universe having a system of non-interacting diffusive cosmic fluids with barotropic equation of state (constant or variable equation of state parameter). Due to diffusive nature of the cosmic fluids, the divergence of the energy momentum tensor is chosen to be proportional to the diffusive current. The thermodynamic stability analysis of individual fluids is done and the stability conditions are expressed as restrictions on the equation of state parameter.
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spelling doaj.art-1b89579a868541eb980decb015b1f5e22022-12-22T01:55:42ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-01-017911810.1140/epjc/s10052-019-6603-0Universe consisting of diffusive dark fluids: thermodynamics and stability analysisSubhayan Maity0Pritikana Bhandari1Subenoy Chakraborty2Department of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityDepartment of Mathematics, Jadavpur UniversityAbstract The present work deals with homogeneous and isotropic FLRW model of the Universe having a system of non-interacting diffusive cosmic fluids with barotropic equation of state (constant or variable equation of state parameter). Due to diffusive nature of the cosmic fluids, the divergence of the energy momentum tensor is chosen to be proportional to the diffusive current. The thermodynamic stability analysis of individual fluids is done and the stability conditions are expressed as restrictions on the equation of state parameter.http://link.springer.com/article/10.1140/epjc/s10052-019-6603-0
spellingShingle Subhayan Maity
Pritikana Bhandari
Subenoy Chakraborty
Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
European Physical Journal C: Particles and Fields
title Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
title_full Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
title_fullStr Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
title_full_unstemmed Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
title_short Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
title_sort universe consisting of diffusive dark fluids thermodynamics and stability analysis
url http://link.springer.com/article/10.1140/epjc/s10052-019-6603-0
work_keys_str_mv AT subhayanmaity universeconsistingofdiffusivedarkfluidsthermodynamicsandstabilityanalysis
AT pritikanabhandari universeconsistingofdiffusivedarkfluidsthermodynamicsandstabilityanalysis
AT subenoychakraborty universeconsistingofdiffusivedarkfluidsthermodynamicsandstabilityanalysis