Accelerating Kerr–Newman black holes in (anti-)de Sitter space-time

J. Podolský, J. B. Griffiths
2006 Physical Review D  
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.
doi:10.1103/physrevd.73.044018 fatcat:3i3rp2lv7zb2xhiey6i3e5frde