An inhomogeneous cosmological model

Details An inhomogeneous cosmological model An inhomogeneous cosmological model

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ukfiz..29..969k&link_type=abstract

Ukrainskii Fizicheskii Zhurnal (ISSN 0503-1265), vol. 29, July 1984, p. 969-977. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Cosmology, Einstein Equations, Gravitation Theory, Inhomogeneity, Macroscopic Equations, Unified Field Theory, Universe

Scientific paper

Some characteristic 'macroscopic' gravitational equations obtained on the basis of the mathematical model of Fisher and Shirokov (1963) are examined. The secondary terms of the equations are correlated with the early stages of the evolution of the universe and are helpful in removing singularities from solutions of macroscopic gravitational equations. Polarization impurities for the case of a 'dustlike' universe are found to be insignificant.

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