Effects of second viscosity in cosmology

Details Effects of second viscosity in cosmology Effects of second viscosity in cosmology

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978svphj..21...76p&link_type=abstract

Soviet Physics Journal, Volume 21, Issue 1, pp.76-81

Physics

Scientific paper

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.

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