Slowly rotating superdense configurations in Rosen's Bimetric Theory of Gravitation

Details Slowly rotating superdense configurations in Rosen's Bimetric Theory of Gravitation Slowly rotating superdense configurations in Rosen's Bimetric Theory of Gravitation

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..98....1c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 98, no. 1, Jan. 1984, p. 1-14.

Astronomy and Astrophysics

Astrophysics

7

Astronomical Models, Bimetric Theories, Gravitation Theory, Rotating Environments, Angular Velocity, Baryons, Differential Equations, Moments Of Inertia

Scientific paper

In the limits of the Bimetric Theory of Gravitation the equations of axial-symmetric gravitational field, describing the field of rotating configurations, are obtained and examined. The analytical solutions of these equations out of configurations are found. The equations are solved numerically in the first approximation in the angular velocity for the configurations consisting of the real baryon gas (cf. Sahakian, 1972). The moments of inertia of these configurations in BTG are calculated. It is shown that the equations and the appropriate solution, obtained by Falik and Opher (1979), are incorrect.

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