Galaxy formation from tepid inflation

Details Galaxy formation from tepid inflation Galaxy formation from tepid inflation

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..347l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 2, July 1988, p. 347-354.

Statistics

Computation

1

Cosmology, Galactic Evolution, Space Density, Computational Astrophysics, Density Distribution, Entropy, Inflating, Perturbation Theory

Scientific paper

The primordial density fluctuations necessary for galaxy formation are modeled as being of thermal origin and in a quasi-exponential state of inflation. Adopting the tepid inflation model, it is shown that 10 to the 87th entropy and 10 to the 29th times expansion appear at 92 percent supercooling for all reasonable Higgs parameters. The present scenario avoids the strongest restriction of inflationary models on cosmological observables.

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