On the singularity in Rosen's bimetric theory of gravitation

Details On the singularity in Rosen's bimetric theory of gravitation On the singularity in Rosen's bimetric theory of gravitation

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..197s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 1, April 1985, p. 197-201.

Mathematics

Bimetric Theories, Gravitation Theory, Magnetohydrodynamics, Metric Space, Relativistic Effects, Singularity (Mathematics), Mass Distribution, Radii, Scalars, Schwarzschild Metric, Tensors

Scientific paper

It is shown that Rosen's bimetric theory of gravitation also has a Schwarzschild-type singularity. The radius of the singularity - the gravitational radius - is defined by the secondary mass M1. Simultaneously it is shown that only those configurations are stable, which are located in the range of central densities corresponding to the increasing branch of the M1 = M1(ρc) curve.

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