Friedmann-Robertson-Walker vacuum solutions in the scale covariant theory

Details Friedmann-Robertson-Walker vacuum solutions in the scale covariant theory Friedmann-Robertson-Walker vacuum solutions in the scale covariant theory

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..415b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 119, no. 2, Feb. 1986, p. 415-420. Research supported by the Council for S

Astronomy and Astrophysics

Astrophysics

9

Cosmology, Covariance, Gravitation Theory, Universe, Vacuum, Astronomical Models, Asymptotic Properties, Scale

Scientific paper

It is shown that the empty Friedmann-Robertson-Walker solutions exhibit much more diverse behavior in the scale-covariant theory than in general relativity. The analysis reveals that the de-Sitter-type universe need not necessarily be expanding, as in the general relativistic case. It is also demonstrated that asymptotic considerations at large cosmological times lead to the Milne and de Sitter solutions in the scale-covariant theory.

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