Dressing up a Kerr naked singularity

Details Dressing up a Kerr naked singularity Dressing up a Kerr naked singularity

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ncimb..51..247c&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 51B, June 11, 1979, p. 247-261. Research supported by the Consiglio Nazionale delle Ricerche.

Astronomy and Astrophysics

Astronomy

7

Black Holes (Astronomy), Singularity (Mathematics), Stellar Evolution, Stellar Mass Accretion, Capture Effect, Gravitational Collapse, Mass Transfer, Space-Time Functions, Stellar Luminosity

Scientific paper

The evolution of a naked singularity surrounded by an accreting disk of matter is studied. Two kinds of disk are considered: the standard thin-disk model and the thick barytropic model, for several initial conditions. It is shown that any Kerr naked singularity slows down in a finite time to a maximal Kerr black hole. The final mass, luminosity, and time of evolution of the singularity are evaluated.

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