Effective ergospheres of magnetized black holes and the Kerr-Newman-Ernst solution

Details Effective ergospheres of magnetized black holes and the Kerr-Newman-Ernst solution Effective ergospheres of magnetized black holes and the Kerr-Newman-Ernst solution

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988zhetf..94q..15a&link_type=abstract

Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0044-4510), vol. 94, Aug. 1988, p. 15-28. In Russian.

Statistics

Computation

2

Black Holes (Astronomy), Charged Particles, Computational Astrophysics, Magnetic Effects, Neutral Particles, Gravitational Fields, Magnetic Fields, Magnetization

Scientific paper

The effective ergospheres of neutral and charged particles near a rotating black hole immersed in an external uniform magnetic field are described. It is shown that the magnetic field alters the chemical potential of the horizon and the entropy of the black hole. It is noted that magnetic entrainment of the reference system around a charged hole in a magnetic field may occur. In the general case, the Harrison transformation leads to conical singularities. A modified Kerr-Newman-Ernst solution, which describes a rotating charged black hole in an external magnetic field, is derived by allowing for the effect of the field on the metric.

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