Statistical fluctuations in an inflationary universe

Details Statistical fluctuations in an inflationary universe Statistical fluctuations in an inflationary universe

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142l..29r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. L29-L31.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Cosmology, Statistical Analysis, Universe, Baryons, Galactic Clusters, Galaxies, Variations

Scientific paper

The applicability of statistical fluctuations as an explanation for the structure of the universe is discussed within the framework of inflationary universe models. Consideration is given to: the effects of fluctuations on the scale of 10 to the 17th solar mass on observational limits to microwave background anisotropies; the time evolution of fluctuations in the models of Friedmann and Zel'dovich (1972); and adiabatic perturbations. The theoretical equations of the models are modified with respect to the statistical fluctuations, and the results are discussed in detail.

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