Transition of rotating Bianchi type-IX cosmological model into an inflationary era

Details Transition of rotating Bianchi type-IX cosmological model into an inflationary era Transition of rotating Bianchi type-IX cosmological model into an inflationary era

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.1204g&link_type=abstract

Physical Review D (Particles and Fields), Volume 33, Issue 4, 15 February 1986, pp.1204-1205

Mathematics

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21

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Scientific paper

A Bianchi type-IX cosmological model has been found as a solution of Einstien's vacuum field equations with a cosmological constant. The solution represents a rotating generalziation fo the de Sitter universe. This universe shows a transition to exponential expansion and the vorticity begins to decay exponentially at the grand-unified-theory time. The point of time for this transition is independent of the magnitude of the vorticity. During the Guth inflationary era the vorticity decays by a factor of the order 10-142.

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