Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2001-12-06
Class.Quant.Grav. 19 (2002) 4553-4564
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
LaTeX 2.09, no figures, 15 pages, v2, references added, introduction section slightly modified; v3, grammar errors corrected
Scientific paper
10.1088/0264-9381/19/17/307
Axially symmetric, stationary solutions of the Einstein-Maxwell equations with disconnected event horizon are studied by developing a method of explicit integration of the corresponding boundary-value problem. This problem is reduced to non-leaner system of algebraic equations which gives relations between the masses, the angular momenta, the angular velocities, the charges, the distance parameters, the values of the electromagnetic field potential at the horizon and at the symmetry axis. A found solution of this system for the case of two charged non-rotating black holes shows that in general the total mass depends on the distance between black holes. Two-Killing reduction procedure of the Einstein-Maxwell equations is also discussed.
Chistyakov A. S.
Varzugin Gennadii
No associations
LandOfFree
Charged Rotating Black Holes in Equilibrium does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Charged Rotating Black Holes in Equilibrium, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Charged Rotating Black Holes in Equilibrium will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-372132