@Article{Babichev+Fabbri2014,
author="Babichev, E.
and Fabbri, A.",
title="Rotating black holes in massive gravity",
journal="Physical Review D",
year="2014",
publisher="Amer Physical Soc",
volume="90",
number="8",
pages="084019--7pp",
abstract="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.",
optnote="WOS:000343773100005",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=1984), last updated on Thu, 27 Nov 2014 12:33:24 +0000",
issn="1550-7998",
doi="10.1103/PhysRevD.90.084019",
opturl="http://arxiv.org/abs/1406.6096",
opturl="https://doi.org/10.1103/PhysRevD.90.084019",
archivePrefix="arXiv",
eprint="1406.6096",
language="English"
}