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Download fileAccelerating Kerr-Newman black holes in (anti-) de Sitter space-time
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posted on 03.02.2006, 11:19 by J. Podolsky, Jerry GriffithsA class of exact solutions of the Einstein–Maxwell equations is presented which describes an accelerating
and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe.
The metric is presented in a new and convenient form in which the meaning of the parameters is
clearly identified, and from which the physical properties of the solution can readily be interpreted.
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