Exterior gravitational field of a charged rotating mass with arbitrary quadrupole moment
Por:
Quevedo H., Mashhoon B.
Publicada:
1 ene 1990
Resumen:
We present a generalization of the exterior charged Kerr spacetime involving an arbitrary spheroidal deformation of the mass. The metric for this stationary axisymmetric solution of the Einstein-Maxwell equations is explicitly given, and some of its physical properties are briefly discussed. © 1990.
Filiaciones:
Quevedo H.:
Institute for Theoretical Physics, University of Cologne, D-5000 Cologne 41, Germany
Mashhoon B.:
Department of Physics and Astronony, University of Missouri-Columbia, Columbia, MO 65211, United States
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