%0 Journal Article
%T Rotating black holes in massive gravity
%A Babichev, E.
%A Fabbri, A.
%J Physical Review D
%D 2014
%V 90
%N 8
%I Amer Physical Soc
%@ 1550-7998
%G English
%F Babichev+Fabbri2014
%O WOS:000343773100005
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=1984), last updated on Thu, 27 Nov 2014 12:33:24 +0000
%X We present a solution for rotating black holes in massive gravity. We first give a solution of massive gravity with one dynamical metric. Both metrics of this solution are expressed in the advanced Eddington-Finkelstein-like coordinates: the physical metric has the original Kerr line element, while the fiducial metric is flat, but written in a rotating Eddington-Finkelstein form. For the bigravity theory we give an analogue of this solution: the two metrics have the original Kerr form, but, in general, different black hole masses. The generalization of the solution to include the electric charge is also given; it is an analogue of the Kerr-Newman solution in general relativity. We also discuss further possible ways to generalize the solutions.
%R 10.1103/PhysRevD.90.084019
%U http://arxiv.org/abs/1406.6096
%U https://doi.org/10.1103/PhysRevD.90.084019
%P 084019-7pp