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Inflation in inhomogeneous cosmology
Phys. Rev. D 45, 2802 – Published 15 April, 1992
DOI: https://doi.org/10.1103/PhysRevD.45.2802
Abstract
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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