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In the context of f(R) theories of gravity, we address the problem of findinga rotating charged black hole solution in the case of constant curvature. Thenew metric is obtained by solving the field equations and we show that thebehavior of it is typical of a rotating charged source. In addition, we analyzethe thermodynamics of the new black hole. The results ensures that thethermodynamical properties in f(R) gravities are qualitatively similar to thoseof standard General Relativity.

A Rotating Charged Black Hole Solution in f(R) Gravity