Astrophysical Black Holes With Spin and Charge

Details Astrophysical Black Holes With Spin and Charge Astrophysical Black Holes With Spin and Charge

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.107d&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Effects of charge and spin on the black hole engines of astrophysical objects are studied in the Kerr-Newman solution of general relativity. A (geometrized) charge e yields more change from the Schwarzschild spacetime than does an equal amount of spin/mass a. Charged black hole fusion produces radiation more efficiently than rotating black hole fusion. Particles on geodesics of Kerr-Newman geometry are repelled at radii which are roots of quartic equations. Clearly, the simpler Schwarzschild, Reissner-Nordstrom, and Kerr behaviors are recovered as special cases. However, the non-linear interactions of mass, charge, and spin produce interesting combined effects which are not intuitive.

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