Quantum formation of black holes and wormholes in the gravitational collapse of a dust shell
- 15 April 1996
- journal article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 53 (8) , 4356-4365
- https://doi.org/10.1103/physrevd.53.4356
Abstract
A quantum-mechanical model of a self-gravitating dust shell is considered. To clarify the relation between classical and quantum spacetime which the shell collapse forms, we consider various time slicings on which quantum mechanics is developed. By considering the static time slicing which corresponds to an observer at a constant circumference radius, we obtain the wave functions of the shell motion and the discrete mass spectra which specify the global structures of spherically symmetric spacetime formed by the shell collapse. It is found that wormhole states are forbidden when the rest mass is comparable to the Planck mass scale due to the zero-point quantum fluctuations. © 1996 The American Physical Society.Keywords
All Related Versions
This publication has 21 references indexed in Scilit:
- Quantum dynamics of Lorentzian spacetime foamPhysical Review D, 1994
- Quantum collapse of a self-gravitating shell: Equivalence to Coulomb scatteringPhysical Review D, 1992
- Quantum mechanics of gravitational collapseCommunications in Mathematical Physics, 1992
- QUANTUM BOUNCE OF A UNIFORM DUST STAR IN NEWTON GRAVITYModern Physics Letters A, 1991
- Quantum wormholesPhysical Review D, 1991
- On a quantum mechanical model of a black holePhysics Letters B, 1990
- On the quantum mechanics of bubblesPhysics Letters B, 1988
- Breakdown of predictability in gravitational collapsePhysical Review D, 1976
- Particle creation by black holesCommunications in Mathematical Physics, 1975
- Singular hypersurfaces and thin shells in general relativityIl Nuovo Cimento B (1971-1996), 1967