Notes on sums over horizons
arXiv:2407.13079 · doi:10.1103/PhysRevD.110.024028
Abstract
For a large class of black holes, we show that the sum of thermodynamic quantities over all the horizons is determined by the asymptotic data at infinity. For the Kerr-Newman metric, this proves a recent numerical observation by Hristov. We propose a new method to compute the sum of the entropies using a generalized Smarr formula. The higher-curvature corrections in Gauss-Bonnet gravity are discussed.
References in corpus (21)
- The Black Hole in Three Dimensional Space Time
- Enthalpy and the Mechanics of AdS Black Holes
- Gauss-Bonnet Black Holes in AdS Spaces
- Thermodynamics of Kerr-Newman-AdS Black Holes and Conformal Field Theories
- The entropy of Hawking radiation
- Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
- Rotation and the AdS/CFT correspondence
- The First Law of Thermodynamics for Kerr-Anti-de Sitter Black Holes
- The General Kerr-de Sitter Metrics in All Dimensions
- P-V criticality in the extended phase space of Gauss-Bonnet black holes in AdS space
- General Non-Extremal Rotating Black Holes in Minimal Five-Dimensional Gauged Supergravity
- Universal Area Product Formulae for Rotating and Charged Black Holes in Four and Higher Dimensions
- Equal charge black holes and seven dimensional gauged supergravity
- Entropy-Product Rules for Charged Rotating Black Holes
- Charged rotating black holes in six-dimensional gauged supergravity
- The "universal property" of Horizon Entropy Sum of Black Holes in Four Dimensional Asymptotical (anti-)de-Sitter Spacetime Background
- A Note on Entropy Relations of Black Hole Horizons
- The Universal Property of the Entropy Sum of Black Holes in All Dimensions
- The Entropy Sum of (A)dS Black Holes in Four and Higher Dimensions
- Thermodynamic relations for entropy and temperature of multi-horizons black holes
- Explicit black hole thermodynamics in natural variables