Black holes or compact stars?

Details Black holes or compact stars? Black holes or compact stars?

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...143l...5h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 143, no. 2, Feb. 1985, p. L5, L6.

Astronomy and Astrophysics

Astronomy

Bimetric Theories, Black Holes (Astronomy), Gravitational Collapse, Relativity, Stellar Structure, Hydrostatics, Schwarzschild Metric, Singularity (Mathematics)

Scientific paper

The structure of a typical star is investigated analytically both in the framework of general relativity (GR) and in the bimetric version of GR developed by Rosen (1980) and Falik and Rosen (1980) to eliminate singularities appearing in the solutions of the Einstein field equations. The results of the two analyses are shown to be identical for an ordinary star, but bimetric GR predicts that a collapsed star which fills its Schwarzschild radius is in hydrostatic equilibrium, while GR predicts continued collapse to a point singularity at the center of a black hole.

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