Accretion disks in the bimetric theory of gravitation - The strong gravity of the inner disk edge

Details Accretion disks in the bimetric theory of gravitation - The strong gravity of the inner disk edge Accretion disks in the bimetric theory of gravitation - The strong gravity of the inner disk edge

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..559c&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Dec. 1987, p. 559-569.

Statistics

Computation

Accretion Disks, Bimetric Theories, Gravitation Theory, Bremsstrahlung, Computational Astrophysics, Optical Thickness

Scientific paper

Optically thin bremsstrahlung accretion disks, calculated in the bimetric theory of gravitation, are compared with the corresponding ones in Einstein's theory. The sensibility of the inner disk edge located in a strong gravity region of the sufficiently compact central object suggests arguments for the confirmation that the accretion disk as a whole could be determined by strong gravity effects.

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