Inflation in a spatially closed anisotropic universe.

Details Inflation in a spatially closed anisotropic universe. Inflation in a spatially closed anisotropic universe.

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jmp....31..371p&link_type=abstract

Journal of Mathematical Physics, Vol. 31, No. 2, p. 371 - 377

Mathematics

Mathematical Physics

9

Cosmology: Inflationary Universe

Scientific paper

The effects of shear on the occurrence of inflation are studied on the basis of a simple model for a spatially closed universe which enters an inflationary era. It is found that the inclusion of (positive) shear retards the occurrence of the vacuum phase transition. The magnitude of this effect depends on the mass of the universe at the time of the phase transition.

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