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Thermodynamic Topological Classes of Family of Black Holes with NUT-Charge

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arxiv 2502.13914 v2 pith:WXHCAFQI submitted 2025-02-19 gr-qc

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keywords thermodynamictopologicalblackclassclassesfamilyholesnut-charge
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{We introduce new analytical methods for treating black-hole thermodynamic topology, and thus depart from the usual treatment known in the literature. As application we investigate the universal thermodynamic topological classes of a family of black holes with NUT-charge. A charge-dependent thermodynamic topological transition from one class to another class is discussed.

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Cited by 1 Pith paper

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  1. High-order QED correction impacts on phase transition of the Euler-Heisenberg dS spacetime

    hep-th 2025-07 conditional novelty 5.0 of 10

    The dual-horizon coexistence region in Euler-Heisenberg de Sitter spacetime exhibits van der Waals-like phase transitions whose order depends on a nonlinear parameter, with a constant topological number W=+1.

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