posted on 2006-02-03, 11:19authored byJ. Podolsky, Jerry Griffiths
A 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.
History
School
Science
Department
Mathematical Sciences
Pages
152797 bytes
Publication date
2006
Notes
This is a pre-print. It is also available at: http://xxx.soton.ac.uk/abs/gr-qc/0601130.