Viscous cosmologies in scalar-tensor theories for Kasner type metrics

Details Viscous cosmologies in scalar-tensor theories for Kasner type metrics Viscous cosmologies in scalar-tensor theories for Kasner type metrics

2000-11-07

arxiv.org/abs/gr-qc/0011027v1

Phys.Rev. D63 (2001) 063503

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, Latex, accepted in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.63.063503

In a viscous Bianchi type I metric of the Kasner form, it is well known that it is not possible to describe an anisotropic physical model of the universe, which satisfies the second law of thermodynamics and the dominant energy condition (DEC) in Einstein's theory of gravity. We examine this problem in scalar-tensor theories of gravity. In this theory we show that it is possible to describe the growth of entropy, keeping the thermodynamics and the dominant energy condition.

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