Expanding Universe with bulk and shear viscosity in conformally flat coordinates View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1978-08

AUTHORS

G. E. Tauber

ABSTRACT

Conformally flat line-elements are applied to imperfect fluids in cosmology. Explicit solutions of the field equations are given for an equation of state for which the pressure is proportional to the density. Both the isotropic case (for which the shear viscosity vanishes) and the non-isotropic case are considered and expressions derived for the appropriate coefficients of shear and bulk viscosity, as well as density. More... »

PAGES

163-179

References to SciGraph publications

  • 1973-01. Imperfect fluid Friedmannian cosmology in ASTROPHYSICS AND SPACE SCIENCE
  • 1970-11. Transport coefficients of a relativistic quantum gas in LETTERE AL NUOVO CIMENTO (1969-1970)
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/bf00639053

    DOI

    http://dx.doi.org/10.1007/bf00639053

    DIMENSIONS

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