Homogeneous Universes in Extended Inflation I

Details Homogeneous Universes in Extended Inflation I Homogeneous Universes in Extended Inflation I

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.249..179g&link_type=abstract

Astrophysics and Space Science, Volume 249, Issue 2, pp.179-188

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We have found that for the Bianchi types I-II-III-V in the Brans-Dicke theory, the scalar field of the theory φ has the same form in the isotropic case. It is shown that the isotropization of the Universe occurs in a very short time when the Universe is dominated by vacuum energy, proving that an isotropic Robertson-Walker model is a good approximation to use in the extended inflation scenario.

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