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Thermodynamic scheme of inhomogeneous perfect fluid mixtures

Rubén D Zárate1 and Hernando Quevedo2

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We analyse the compatibility between the geometrodynamics and thermodynamics of a binary mixture of perfect fluids which describe inhomogeneous cosmological models. We generalize the thermodynamic scheme of general relativity to include the chemical potential of the fluid mixture with non-vanishing entropy production. This formalism is then applied to the case of Szekeres and Stephani families of cosmological models. The compatibility conditions turn out to impose symmetry conditions on the cosmological models in such a way that only the limiting case of the Friedmann–Robertson–Walker model remains compatible. This result is an additional indication of the incompatibility between thermodynamics and relativity.


PACS

05.70.-a Thermodynamics

98.80.Jk Mathematical and relativistic aspects of cosmology

04.20.-q Classical general relativity

04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields

MSC

83Cxx General relativity

85A40 Cosmology (For relativistic cosmology, see 83F05)

82B30 Statistical thermodynamics (See also 80-XX)

83F05 Cosmology

83E05 Geometrodynamics

Subjects

Gravitation and cosmology

Statistical physics and nonlinear systems

Astrophysics and astroparticles

Dates

Issue 1 (7 January 2004)

Received 22 August 2003

Published 20 November 2003



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