Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2007-11-28
Phys.Rev.D77:104022,2008
Physics
High Energy Physics
High Energy Physics - Theory
9 pages, 7 figures, references added, to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.77.104022
We present a new class of slowly rotating black hole solutions in $(n+1)$-dimensional $(n\geq3)$ Einstein-Maxwell-dilaton gravity in the presence of Liouville-type potential for the dilaton field and an arbitrary value of the dilaton coupling constant. Because of the presence of the dilaton field, the asymptotic behaviour of these solutions are neither flat nor (A)dS. In the absence of a dilaton field, our solution reduces to the $(n+1)$-dimensional Kerr-Newman modification thereof for small rotation parameter \cite{Aliev2}. We also compute the angular momentum and the gyromagnetic ratio of these rotating dilaton black holes.
No associations
LandOfFree
Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotating Black Holes in Einstein-Maxwell-Dilaton Gravity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-248693