Rotating Black Holes: NUT charges and effective Kerr Variants

This doctoral thesis focuses on the exploration of Kerr black holes and their thermodynamic properties, with the aim of broadening our understanding of these fascinating entities from the perspective of theoretical physics. The thesis is structured into two clearly differentiated chapters, in which a thermodynamic study is conducted on two types of rotating black holes: Kerr–Taub-NUT AdS black holes within the framework of General Relativity, and the so-called Kerr Effective Geometries, which arise as solutions in N=2 Supergravity.

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IFT