Relativistic Formulation and Cosmological Applications

  • David Jou
  • José Casas-Vázquez
  • Georgy Lebon

Abstract

The attention paid to dissipative phenomena in cosmology and astrophysics is growing steadily. The interaction between matter and radiation leads to dissipative effects which are of importance for the evolution of the Universe and the survival of protogalaxies. In astrophysics, the thermal conductivity and the viscosity of a gas of neutrinos play a role in phenomena like stellar collapse. In cosmology, bulk viscosity provides a source of dissipation which may have relevant effects on the dynamics of the Universe. These have fostered the research on relativistic non-equilibrium thermodynamic theories.

Keywords

Entropy Microwave Anisotropy Recombination Nism 

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Copyright information

© Springer-Verlag Berlin Heidelberg 1996

Authors and Affiliations

  • David Jou
    • 1
  • José Casas-Vázquez
    • 1
  • Georgy Lebon
    • 2
  1. 1.Departament de FísicaUniversitat Autònoma de Barcelona, Grup de Física EstadísticaBellaterra, CataloniaSpain
  2. 2.Département de PhysiqueUniversité de LiègeLiègeBelgium

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