Quantum superposition principle and gravitational collapse: Scattering times for spherical shells
arXiv:gr-qc/0507017 · doi:10.1103/PhysRevD.72.064025
Abstract
A quantum theory of spherically symmetric thin shells of null dust and their gravitational field is studied. In Nucl. Phys. 603 (2001) 515 (hep-th/0007005), it has been shown how superpositions of quantum states with different geometries can lead to a solution of the singularity problem and black hole information paradox: the shells bounce and re-expand and the evolution is unitary. The corresponding scattering times will be defined in the present paper. To this aim, a spherical mirror of radius R_m is introduced. The classical formula for scattering times of the shell reflected from the mirror is extended to quantum theory. The scattering times and their spreads are calculated. They have a regular limit for R_m\to 0 and they reveal a resonance at E_m = c^4R_m/2G. Except for the resonance, they are roughly of the order of the time the light needs to cross the flat space distance between the observer and the mirror. Some ideas are discussed of how the construction of the quantum theory could be changed so that the scattering times become considerably longer.
30 pages and 5 figures; the post-referee version: shortened and some formulations improved; to be published in Physical Review
Cited by in corpus (24)
- Black hole fireworks: quantum-gravity effects outside the horizon spark black to white hole tunneling
- Phenomenological aspects of black holes beyond general relativity
- White Holes as Remnants: A Surprising Scenario for the End of a Black Hole
- Classical collapse to black holes and quantum bounces: A review
- Singularity avoidance for collapsing quantum dust in the Lemaitre-Tolman-Bondi model
- Where does the physics of extreme gravitational collapse reside?
- Black holes turn white fast, otherwise stay black: no half measures
- Exponential fading to white of black holes in quantum gravity
- Towards a quantum Oppenheimer-Snyder model
- Role of evaporation in gravitational collapse
- Classical mass inflation vs semiclassical inner horizon inflation
- Quantum Oppenheimer-Snyder model
- Quantum self-gravitating collapsing matter in a quantum geometry
- Exteriors to bouncing collapse models
- Entropy of extremal black holes: horizon limits through charged thin shells, a unified approach
- Diffuse emission from black hole remnants
- Black hole evolution in quantum-gravitational framework
- Numerical approach to the black-to-white hole transition
- Semi-Classical Holomorphic Transition Amplitudes in Covariant Loop Quantum Gravity
- A predictive framework for quantum gravity and black hole to white hole transition
- Infrared signatures of quantum bounce in a minisuperspace analysis of Lema\^ıtre-Tolman-Bondi dust collapse
- Wheeler-DeWitt equation and the late gravitational collapse: effects of factor ordering and the tunneling scenario
- Dynamics of a self gravitating light-like matter shell with spherical symmetry
- Collapsing Layers on Schwarzschild-Lemaitre Geodesics