2026-07-29T01:54:05Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/427552023-08-26T08:36:56Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Jimeno Romero, Pablo
author
Ruiz Cembranos, José Alberto
author
Cruz Dombriz, Álvaro de la
2023-06-20T00:34:40Z
2023-06-20T00:34:40Z
2012-07
0094-243x
10.1063/1.4734454
https://hdl.handle.net/20.500.14352/42755
http://dx.doi.org/10.1063/1.4734454
http://aip.scitation.orghttp://arxiv.org/abs/1202.0853
In the context of f(R) modified gravity theories we determine that the black holes existence is determined by the sign of a parameter dependent of the mass, the charge, the spin and the scalar curvature. We obtain the different astrophysical objects derived from the presence of different horizons. Thermodynamics for this kind of black holes is studied for negative values of the curvature, revealing that we can distinguish between two kind of BH: fast and slow.
eng
Modified spinning black holes
journal article
URL
https://docta.ucm.es/bitstreams/12e1a2c2-7c8e-4ae8-a656-12342b830b30/download
File
MD5
784dcedb7fbd0828d070aba3532a1058
195951
application/pdf
Cembranos,JAR15.pdf