The third law of black hole thermodynamics and the mass-to-charge ratio of scalar fields
gr-qc, astro-ph.HE, hep-th
Submitted: 2026-09-24
Updated: 2026-09-24
Terminology
Sources
- Gravitational collapse to extremal black holes and the third law of black hole thermodynamics
- Formation of extremal Reissner-Nordstr\"om black holes: insights from numerics
- Universal Bound on Dynamical Relaxation Times and Black-Hole Quasinormal Ringing
- Near-Extreme Black Holes and the Universal Relaxation Bound
- Quasinormal resonances of near-extremal Kerr-Newman black holes
- Slow relaxation of rapidly rotating black holes
- Black-hole quasinormal resonances: Wave analysis versus a geometric-optics approximation
- Quasinormal resonances of rapidly-spinning Kerr black holes and the universal relaxation bound
- The third law of black hole thermodynamics: Quantum versus classical considerations
- Spontaneous Pair Production in Reissner-Nordstrom Black Holes
- A third law of black hole mechanics for supersymmetric black holes and a quasi-local mass-charge inequality
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