Quantum Hair on Colliding Black Holes
@article{Crowell2020QuantumHO, title={Quantum Hair on Colliding Black Holes}, author={Lawrence Barr Crowell and Christian Corda}, journal={Entropy}, year={2020}, volume={22} }
Black hole (BH) collisions produce gravitational radiation which is generally thought, in a quantum limit, to be gravitons. The stretched horizon of a black hole contains quantum information, or a form of quantum hair, which is a coalescence of black holes participating in the generation of gravitons. This may be facilitated with a Bohr-like approach to black hole (BH) quantum physics with quasi-normal mode (QNM) approach to BH quantum mechanics. Quantum gravity and quantum hair on event…
2 Citations
References
SHOWING 1-10 OF 55 REFERENCES
Quantum Black Holes as Atoms
- Physics
- 1997
In some respects the black hole plays the same role in gravitation that the atom played in the nascent quantum mechanics. This analogy suggests that black hole mass $M$ might have a discrete…
Black hole explosions?
- PhysicsNature
- 1974
QUANTUM gravitational effects are usually ignored in calculations of the formation and evolution of black holes. The justification for this is that the radius of curvature of space-time outside the…
Quasi-Normal Modes: The “Electrons” of Black Holes as “Gravitational Atoms”? Implications for the Black Hole Information Puzzle
- Physics
- 2015
Some recent important results on black hole (BH) quantum physics concerning the BH effective state and the natural correspondence between Hawking radiation and BH quasi-normal modes (QNMs) are…
Hawking Radiation-Quasinormal Modes Correspondence for Large AdS Black Holes
- Physics
- 2017
It is well-known that the nonstrictly thermal character of the Hawking radiation spectrum generates a natural correspondence between Hawking radiation and black hole quasinormal modes. This main…
Information in black hole radiation.
- PhysicsPhysical review letters
- 1993
If black hole formation evaporation can be described by an S matrix, information would be expected to come out in black hole radiation. An estimate shows that it may come out initially so slowly, or…
Extremal limits and black hole entropy
- Physics
- 2009
Taking the extremal limit of a non-extremal Reissner-Nordstrom black hole (by externally varying the mass or charge), the region between the inner and outer event horizons experiences an interesting…
Black holes: complementarity or firewalls?
- Physics
- 2012
A bstractWe argue that the following three statements cannot all be true: (i) Hawking radiation is in a pure state, (ii) the information carried by the radiation is emitted from the region near the…
The Large-N Limit of Superconformal Field Theories and Supergravity
- Physics, Mathematics
- 1997
We show that the large-N limits of certainconformal field theories in various dimensions includein their Hilbert space a sector describing supergravityon the product of anti-de Sitter spacetimes,…