Inflation in inhomogeneous cosmology

Details Inflation in inhomogeneous cosmology Inflation in inhomogeneous cosmology

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..45.2802c&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 45, Issue 8, 15 April 1992, pp.2802-2805

Physics

35

Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

We discuss the onset of inflation in an inhomogeneous, asymptotically
Friedmann-Robertson-Walker universe coupled to a scalar inflaton field.
We consider a three-parameter family of inhomogeneous Cauchy data, for
which we can solve analytically the constraint equations. Inflation only
occurs if the Cauchy data are homogeneous over several horizon lengths.

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