Rotating polytropic configurations in the bimetric theory of gravitation

Details Rotating polytropic configurations in the bimetric theory of gravitation Rotating polytropic configurations in the bimetric theory of gravitation

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..280c&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, Mar.-Apr. 1981, p. 280-288. In Russian.

Physics

2

Angular Velocity, Bimetric Theories, Field Theory (Physics), Gravitation Theory, Polytropic Processes, Rotating Matter, Astronomical Models, Gravitational Fields, Moments Of Inertia, Relativistic Effects, Stellar Models, Tensor Analysis

Scientific paper

The field equations are solved in the case of the axisymmetric distribution of matter in the bimetric theory of gravitation. The equations are solved numerically in the first approximation in angular velocity for configurations that are described by the polytropic equation of state. The integral characteristics and the internal structure are calculated for configurations with polytropic indices of n = 1, 1.5, 2, 2.5, and 3, and for various values of the relativistic parameter alpha.

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