๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Extended Inflationary Cosmology

โœ Scribed by La, Daile; Steinhardt, Paul J.


Book ID
125524709
Publisher
The American Physical Society
Year
1989
Tongue
English
Weight
209 KB
Volume
62
Category
Article
ISSN
0031-9007

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โœฆ Synopsis


We present a new type of inflationary scenario based on metric formulations of gravity diA'erent from that of Einstein, e.g. , a Brans-Dicke theory of gravity. 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.


๐Ÿ“œ SIMILAR VOLUMES


Extended Inflationary Cosmology
โœ La, Daile; Steinhardt, Paul J. ๐Ÿ“‚ Article ๐Ÿ“… 1989 ๐Ÿ› The American Physical Society ๐ŸŒ English โš– 209 KB
Inflationary cosmology
โœ S Mallik ๐Ÿ“‚ Article ๐Ÿ“… 1993 ๐Ÿ› Springer-Verlag ๐ŸŒ English โš– 499 KB
Inflationary cosmology
โœ Steigman, Gary ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 328 KB
Supersymmetric inflationary cosmology
โœ R. Holman; P. Ramond; G.G. Ross ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 318 KB
Diffusive inflationary cosmology
โœ David D. Bleecker ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 919 KB

In the paradigm of inflation, at some time the early universe behaves roughly as the de Sitter solution of the relativistically covariant (i.e. hyperbolic) vacuum Einstein field equations with a large positive cosmological constant. Here, we consider what happens if a metric g(t) on a compact 3-mani