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oai:docta.ucm.es:20.500.14352/427552023-08-26T08:36:56Zcom_20.500.14352_14col_20.500.14352_15

Jimeno Romero, Pablo Ruiz Cembranos, José Alberto 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.org http://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 open access Modified spinning black holes journal article