Nonthermal nature of extremal Kerr black holes
arXiv:gr-qc/0006036 · doi:10.1016/S0375-9601(00)00515-6
Abstract
Liberati, Rothman and Sonego have recently showed that objects collapsing into extremal Reissner-Nordstrom black holes do not behave as thermal objects at any time in their history. In particular, a temperature, and hence thermodynamic entropy, are undefined for them. I demonstrate that the analysis goes through essentially unchanged for Kerr black holes.
Latex file, 8 pages This post corrects several misprints
References in corpus (1)
Cited by in corpus (15)
- Instability of Extremal Relativistic Charged Spheres
- Extreme Hawking Radiation
- Accelerating boundary analog of a Kerr black hole
- Quantum power distribution of relativistic acceleration radiation: classical electrodynamic analogies with perfectly reflecting moving mirrors
- Extremal Black holes and the limits of the third law
- Hawking radiation particle spectrum of a Kerr-Newman black hole
- On the duality of Schwarzschild-de Sitter spacetime and moving mirror
- Radiation from an inertial mirror horizon
- Relativistic quantum information as radiation reaction: entanglement entropy and self-force of a moving mirror analog to the CGHS black hole
- Möbius Mirrors
- Light and Airy: a simple solution for relativistic quantum acceleration radiation
- Quantum power: a Lorentz invariant approach to Hawking radiation
- Moving mirrors and event horizons in non-flat background geometry
- There and Back Again: Quantum Radiation from Round-trip Flying Mirrors
- Quantum communication through a partially reflecting accelerating mirror