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Thermodynamical Description of Modified Generalized Chaplygin Gas Model of Dark Energy

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Abstract

We consider a universe filled by a modified generalized Chaplygin gas together with a pressureless dark matter component. We get a thermodynamical interpretation for the modified generalized Chaplygin gas confined to the apparent horizon of FRW universe, whiles dark sectors do not interact with each other. Thereinafter, by taking into account a mutual interaction between the dark sectors of the cosmos, we find a thermodynamical interpretation for interacting modified generalized Chaplygin gas. Additionally, probable relation between the thermal fluctuations of the system and the assumed mutual interaction is investigated. Finally, we show that if one wants to solve the coincidence problem by using this mutual interaction, then the coupling constants of the interaction will be constrained. The corresponding constraint is also addressed. Moreover, the thermodynamic interpretation of using either a generalized Chaplygin gas or a Chaplygin gas to describe dark energy is also addressed throughout the paper.

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Acknowledgments

We are grateful to the anonymous reviewers, for valuable comments. The work of H. M. has been supported financially by Research Institute for Astronomy & Astrophysics of Maragha (RIAAM). Under research project No. 1/4165-2.

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Authors and Affiliations

  1. Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran

    H. Ebadi & H. Moradpour

  2. Astrophysics Department, Physics Faculty, University of Tabriz, Tabriz, Iran

    H. Ebadi

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  1. H. Ebadi
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  2. H. Moradpour
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Correspondence to H. Moradpour.

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Ebadi, H., Moradpour, H. Thermodynamical Description of Modified Generalized Chaplygin Gas Model of Dark Energy. Int J Theor Phys 55, 1612–1621 (2016). https://doi.org/10.1007/s10773-015-2799-4

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