Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.
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Topological numbers categorize black hole systems into universality classes based on thermodynamic behavior, with calculations for critical points and phase transitions.
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Hidden Symmetries and Gyromagnetic Ratio of Kerr-Newman Black Holes in $f(R)$ Gravity
Kerr-Newman black holes in f(R) gravity retain the same hidden symmetries and universal gyromagnetic ratio g=2 as in general relativity.
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Topology of black hole thermodynamics: A brief review
Topological numbers categorize black hole systems into universality classes based on thermodynamic behavior, with calculations for critical points and phase transitions.