Asymptotically non-flat rotating dilaton black holes. (English) Zbl 1035.83017
Summary: Dilaton black-hole solutions which are neither asymptotically flat nor (anti-) de Sitter but reduce to asymptotically flat solutions in some special limits have been known for a Liouville-type dilatonic potential. It is shown how, by solving a pair of coupled differential equations, infinitesimally small angular momentum can be added to these static solutions to produce rotating black-hole solutions.
MSC:
83C57 | Black holes |
83E30 | String and superstring theories in gravitational theory |
83C15 | Exact solutions to problems in general relativity and gravitational theory |