2019
DOI: 10.1140/epjc/s10052-019-6603-0
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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 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… Show more

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Cited by 11 publications
(9 citation statements)
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References 40 publications
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“…Only complex scalar field following the restrictions may be the suitable candidate for thermodynamically stable Universe. Also the dark energy (ω < 0) with constant equation of state will not be thermodynamically stable in perturbed universe and this result agrees with previous works on stability criteria of cosmic fluid [31,32].…”
Section: Discussionsupporting
confidence: 92%
See 1 more Smart Citation
“…Only complex scalar field following the restrictions may be the suitable candidate for thermodynamically stable Universe. Also the dark energy (ω < 0) with constant equation of state will not be thermodynamically stable in perturbed universe and this result agrees with previous works on stability criteria of cosmic fluid [31,32].…”
Section: Discussionsupporting
confidence: 92%
“…Within an isolated system which undergoes thermodynamic work done due to the continuous expansion of volume, a stable fluid must possess the positive values of all these thermodynamic derivatives i.e. [31,32]…”
Section: Emergence Of Cosmic Space and Entropy Correction 2nd Lawmentioning
confidence: 99%
“…The elite strategy is to keep the excellent individuals in the parent generation to enter the child generation directly, so as to prevent the loss of Pareto optimal solution [14]. The elite strategy selection operator optimizes the population R i composed of the parent C i , the child D i and the composite R i according to three indexes to form the new parent C i + 1.…”
Section: Methodsmentioning
confidence: 99%
“…The thermodynamical aspects of FRW model of universe with dissipative phenomenon related to effective bulk viscus pressure has been investigated recently [79]. Maity et al [80] have studied the thermodynamic stability of FRW universe having a system of non-interacting diffusive fluids with variable equation of state parameter. It would be interesting to study the behaviour of energy conditions and parameters of expanding universe as par emergent law in the framework of f (R, T ) gravity with particle creation and variable chaplygin gas.…”
Section: Model-iimentioning
confidence: 99%