English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We consider a universe filled by a modified generalized Chaplygin gastogether with a pressureless dark matter component. We get a thermodynamicalinterpretation for the modified generalized Chaplygin gas confined to theapparent horizon of FRW universe, whiles dark sectors do not interact with eachother. Thereinafter, by taking into account a mutual interaction between thedark sectors of the cosmos, we find a thermodynamical interpretation forinteracting modified generalized Chaplygin gas. Additionally, probable relationbetween the thermal fluctuations of the system and the assumed mutualinteraction is investigated. Finally, we show that if one wants to solve thecoincidence problem by using this mutual interaction, then the couplingconstants of the interaction will be constrained. The corresponding constraintis also addressed. Moreover, the thermodynamic interpretation of using either ageneralized Chaplygin gas or a Chaplygin gas to describe dark energy is alsoaddressed throughout the paper.

Thermodynamical description of modified generalized Chaplygin gas model of dark energy