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Soviet Physics Journal

, Volume 21, Issue 1, pp 76–81 | Cite as

Effects of second viscosity in cosmology

  • A. S. Potupa
Article

Abstract

It is shown that in homogeneous cosmological models which take viscosity into account there exist solutions realizing an interpolation between the Friedmann and stationary (steady-state) regimes. In a closed model a solution is obtained which corresponds to the regime of “compensation of curvature” (with radius increasing without bound). The problem of compensation of the singularity as t → 0 and also the choice of equations of state for early (hadron) stages of cosmological evolution in connection with the hydrodynamical theory of multiple creation of hadrons are discussed.

Keywords

Viscosity Cosmological Model Closed Model Cosmological Evolution Hydrodynamical Theory 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Plenum Publishing Corporation 1978

Authors and Affiliations

  • A. S. Potupa
    • 1
  1. 1.V. I. Lenin Belorussian State UniversityUSSR

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