2014/06/30 by Eugeny Babichev, Alessandro Fabbri · 2 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Computer science #Cosmology and Gravitation Theories #Finkelstein's test #General relativity #Generalization #Gravitation #Kerr metric #Massive gravity #Mathematical analysis #Mathematical physics #Mathematics #Metric (unit) #Physics #Pulsars and Gravitational Waves Research #Rotating black hole #Schwarzschild metric #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.90.084019
published as Phys. Rev. D 90, 084019 (2014) · 7 pages; v2: typos corrected, references added; v3: matches published version
openalex publication_date 2014/10/13 · arxiv created 2014/10/29 · arxiv updated 2014/11/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.