Speaker
Ernesto Contreras
(Universidad San Francisco de Quito)
Description
This talk shows a general procedure to construct hairy rotating black holes by deforming a spherically symmetric solution following the Gravitational Decoupling approach. We demonstrate that, in comparison with the well-known Newman-Janis algorithm (with and without complexification), the application of our protocol is straightforward. We provide a particular example of a solution that reduces to the Kerr one, once the primary hair associated with it is turned off.
| Poster fallback option for rejected abstracts for parallel oral presentations | No |
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Author
Ernesto Contreras
(Universidad San Francisco de Quito)
Co-authors
Jorge Ovalle
(Research Centre of Theoretical Physics and Astrophysics, Institute of Physics, Silesian University in Opava, CZ-746 01 Opava, Czech Republic.)
Roberto Casadio
(Dipartimento di Fisica e Astronomia, Alma Mater Universit`a di Bologna, 40126 Bologna, Italy Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, 40127 Bologna, Italy)
