Extended inflationary cosmology

Details Extended inflationary cosmology Extended inflationary cosmology

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..62..376l&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 62, Jan. 23, 1989, p. 376-378.

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Computation

694

Astronomical Models, Cosmology, Gravitation Theory, Space-Time Functions, Computational Astrophysics, Relativistic Theory, Universe, Vacuum

Scientific paper

A new type of inflationary scenario based on metric formulations of gravity different from that of Einstein, e.g., a Brans-Dicke theory of gravity is presented. Unlike previous inflation models, the inflationary phase transition can be completed via bubble nucleation. Hence, the fine tuning of an effective potential to obtain a slow-rollover transition is not required.

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