Journal
MODERN PHYSICS LETTERS A
Volume 32, Issue 13, Pages -Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD
DOI: 10.1142/S021773231750078X
Keywords
Thermodynamic equilibrium; universe expansion; dark energy; dark matter
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Funding
- Research Institute for Astronomy & Astrophysics of Maragha (RIAAM) [1/4165-7]
- CNPq (Conselho Nacional de Desenvolvimento Cientifico e Tecnologico)
- Brazilian scientific support federal agency [302155/2015-5, 302156/2015-1, 442369/2014-0]
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We investigate the relation between the Friedmann and thermodynamic pressure equations, through solving the Friedmann and thermodynamic pressure equations simultaneously. Our investigation shows that a perfect fluid, as a suitable solution for the Friedmann equations leading to the standard modeling of the universe expansion history, cannot simultaneously satisfy the thermodynamic pressure equation and those of Friedmann. Moreover, we consider various energy definitions, such as the Komar mass, and solve the Friedmann and thermodynamic pressure equations simultaneously to get some models for dark energy fluids. The cosmological consequences of obtained solutions are also addressed. Our results indicate that some of obtained solutions may unify the dominated fluid in both the primary inflationary and current accelerating eras into one model. In addition, by taking into account a cosmic fluid of a known equation of state (EoS), and combining it with the Friedmann and thermodynamic pressure equations, we obtain the corresponding energy of these cosmic fluids and face their limitations. Finally, we point out the cosmological features of this cosmic fluid and also study its observational constraints.
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