Tilted Bianchi type-V cosmological model in the scale-covariant theory

Details Tilted Bianchi type-V cosmological model in the scale-covariant theory Tilted Bianchi type-V cosmological model in the scale-covariant theory

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.125...99b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 125, no. 1, Aug. 1986, p. 99-102. Research supported by the Council for Sc

Astronomy and Astrophysics

Astrophysics

11

Cosmology, Gravitation Theory, Gravitational Constant, Differential Equations, Relativity

Scientific paper

Tilted Bianchi type-V solutions in the scale covariant theory of Canuto
et al., (1977) are investigated. The Bianchi type-V model generalizes
the open k = -1 Friedmann model, and it represents a model in which the
fluid flow is not necessarily orthogonal to the three-surfaces of
homogeneity. Both radiative and nonradiative cases are considered.

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