Extending the generalized Chaplygin gas model by using geometrothermodynamics

We use the formalism of geometrothermodynamics (GTD) to derive fundamental thermodynamic equations that are used to construct general relativistic cosmological models. In particular, we show that the simplest possible fundamental equation, which corresponds in GTD to a system with no internal thermo...

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Veröffentlicht in:arXiv.org 2012-09
Hauptverfasser: Aviles, Alejandro, Bastarrachea-Almodovar, Aztlán, Campuzano, Lorena, Quevedo, Hernando
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Quevedo, Hernando
description We use the formalism of geometrothermodynamics (GTD) to derive fundamental thermodynamic equations that are used to construct general relativistic cosmological models. In particular, we show that the simplest possible fundamental equation, which corresponds in GTD to a system with no internal thermodynamic interaction, describes the different fluids of the standard model of cosmology. In addition, a particular fundamental equation with internal thermodynamic interaction is shown to generate a new cosmological model that correctly describes the dark sector of the Universe and contains as a special case the generalized Chaplygin gas model.
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subjects Astronomical models
Chaplygin gas
Computational fluid dynamics
Cosmology
Physics - Cosmology and Nongalactic Astrophysics
Physics - General Relativity and Quantum Cosmology
Universe
title Extending the generalized Chaplygin gas model by using geometrothermodynamics
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