Early stages of the evolution of spatially inhomogeneous models of the universe

Details Early stages of the evolution of spatially inhomogeneous models of the universe Early stages of the evolution of spatially inhomogeneous models of the universe

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979zhetf..77..785p&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki, vol. 77, Sept. 1979, p. 785-800. In Russian.

Astronomy and Astrophysics

Astronomy

2

Astronomical Models, Cosmology, Universe, Einstein Equations, Inhomogeneity, Isotropic Media, Vorticity

Scientific paper

The evolution of spatially inhomogeneous models of the universe is examined at times for which the characteristic size of the inhomogeneity significantly exceeds the size of the event horizon. A mathematical model of an isolated spatial inhomogeneity nested in Friedmann space is presented in the context of density wave theory. It is shown that the presence at the quasi-Friedmann stage of purely spiral motions leads at t greater than 0 to the appearance of potential motions, induced by the redistribution of matter in the inhomogeneity.

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