The degree of generality of inflationary solutions in cosmological models with a scalar field

Details The degree of generality of inflationary solutions in cosmological models with a scalar field The degree of generality of inflationary solutions in cosmological models with a scalar field

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987zhetf..93..784b&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 93, Sept. 1987, p. 784-799. In Russian.

Astronomy and Astrophysics

Astronomy

24

Astronomical Models, Big Bang Cosmology, Anisotropy, Isotropy, Scalars

Scientific paper

The ratio of noninflationary solutions to the total number of solutions
in open and closed Friedmann models and in a homogeneous type I model is
estimated. For the type I and open Friedmann models, the ratio is m/mp,
which is the same as that in the plane Friedmann model. For the closed
Friedmann model, it amounts to 1/4.

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