Force-free fields in the vicinity of a Reissner-Nordstrom black hole

Details Force-free fields in the vicinity of a Reissner-Nordstrom black hole Force-free fields in the vicinity of a Reissner-Nordstrom black hole

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..56..255e&link_type=abstract

Astrophysics and Space Science, vol. 56, no. 1, June 1978, p. 255-269.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Black Holes (Astronomy), Force-Free Magnetic Fields, Electric Potential, Schwarzschild Metric, Spherical Harmonics, Sturm-Liouville Theory, Tensor Analysis

Scientific paper

The behavior of a force-free field has been studied in the Reissner-Nordstrom metric. An expansion in tensor harmonics of even-odd parity reduced the radial equations in a differential equation of the Sturm-Liouville system, which was solved asymptotically in a conveniently defined spatial coordinate. Further, it has been possible to regularize the singular behavior of the Reissner-Nordstrom metric at the event horizon and to specify the modified metric explicitly.

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