Hawking radiation particle spectrum of a Kerr-Newman black hole
DOI10.1088/1475-7516/2021/01/019zbMath1484.83063arXiv2006.09681OpenAlexW3122329627MaRDI QIDQ5025265
Joshua Foo, Michael R. R. Good
Publication date: 1 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2006.09681
Black holes (83C57) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Einstein-Maxwell equations (83C22) Minkowski geometries in nonlinear incidence geometry (51B20)
Related Items (2)
Cites Work
- Last gasp of a black hole: unitary evaporation implies non-monotonic mass loss
- Particle creation by black holes
- Charged particles' tunnelling from the Kerr-Newman black hole
- Microscopic origin of the Bekenstein-Hawking entropy
- On horizonless temperature with an accelerating mirror
- Information preservation for null shell collapse: a moving mirror model
- Entanglement harvesting with moving mirrors
- Time evolution of entanglement entropy of moving mirrors influenced by strongly coupled quantum critical fields
- Recalculation of the spectrum of the radiation emitted during gravitational collapse
- Signatures of energy flux in particle production: a black hole birth cry and death gasp
- Effects of horizons on entanglement harvesting
- Energy associated with a Kerr-Newman black hole
- Onset and decay of the 1 + 1 Hawking–Unruh effect: what the derivative-coupling detector saw
- Radiation from a moving mirror in two dimensional space-time: conformal anomaly
- Radiation from accelerated mirrors following prescribed relativistic asymptotically inertial trajectories
- Radiation from perfect mirrors starting from rest and accelerating forever and the black body spectrum
- Accelerating boundary analog of a Kerr black hole
- Non-existence of isometry-invariant Hadamard states for a Kruskal black hole in a box and for massless fields on 1+1 Minkowski spacetime with a uniformly accelerating mirror
- Hawking Radiation As Tunneling
- Quantum Fields in Curved Space
This page was built for publication: Hawking radiation particle spectrum of a Kerr-Newman black hole