TY  - JOUR
AU  - Babichev, E.
AU  - Fabbri, A.
PY  - 2014
DA  - 2014//
TI  - Rotating black holes in massive gravity
T2  - Phys. Rev. D
JO  - Physical Review D
SP  - 084019
EP  - 7pp
VL  - 90
IS  - 8
PB  - Amer Physical Soc
AB  - 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.
SN  - 1550-7998
UR  - http://arxiv.org/abs/1406.6096
UR  - https://doi.org/10.1103/PhysRevD.90.084019
DO  - 10.1103/PhysRevD.90.084019
LA  - English
N1  - WOS:000343773100005
ID  - Babichev+Fabbri2014
ER  -