Texture and inflation in a closed universe

Details Texture and inflation in a closed universe Texture and inflation in a closed universe

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phrvd..48..943h&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 48, Issue 2, 15 July 1993, pp.943-945

Mathematics

Logic

1

Particle-Theory And Field-Theory Models Of The Early Universe, Unified Theories And Models Of Strong And Electroweak Interactions

Scientific paper

We present a cosmological model with a global homogeneous texture and inflation, but without an initial singularity. The Universe starts from an equilibrium configuration in a symmetric vacuum; the dynamic stability of this configuration is studied. We obtain numerical solutions which show that the Universe expands exponentially and the texture field decays in a finite time; this corresponds to a period of inflation followed naturally by a Friedmann expansion.

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