Evolution of Szekeres's cosmological models

Details Evolution of Szekeres's cosmological models Evolution of Szekeres's cosmological models

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175...85b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, Apr. 1976, p. 85-93.

Astronomy and Astrophysics

Astronomy

47

Astronomical Models, Cosmic Dust, Cosmology, Anisotropic Media, Differential Equations, Einstein Equations, Vector Analysis

Scientific paper

The models are solutions of Einstein's equations for dust with no Killing vectors. They depend on four arbitrary functions of one variable, and generalize both the Friedmann models and those of Kantowski and Sachs (1966). The possibilities of evolution are diverse. One result is that a Friedmann open model can evolve from a variety of initial states, depending on three arbitrary functions of one variable.

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