06-08.pdf (149.22 kB)
Accelerating Kerr-Newman black holes in (anti-) de Sitter space-time
preprintposted on 2006-02-03, 11:19 authored by J. 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.
- Mathematical Sciences
NotesThis is a pre-print. It is also available at: http://xxx.soton.ac.uk/abs/gr-qc/0601130.