Formation of a black hole in the center of a nondissipative gravitational singularity

Details Formation of a black hole in the center of a nondissipative gravitational singularity Formation of a black hole in the center of a nondissipative gravitational singularity

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990zhetf..97...20g&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 97, Jan. 1990, p. 20-31. In Russian.

Statistics

Computation

13

Black Holes (Astronomy), Gravitational Fields, Singularity (Mathematics), Stellar Evolution, Baryons, Computational Astrophysics, Density Distribution, Hydrogen

Scientific paper

The combined dynamics of baryonic and nondissipative matter is examined. The conditions for the appearance of a nondissipative gravitational singularity (NGS) are determined, showing that the emission of energy together with the activity of the gravitational field in the center of the NGS result in an enhanced spherical compression of the baryonic matter. Ultimately, this leads to the formation of a massive black hole which grows rapidly due to the accretion of the baryonic and the nondissipative matter.

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