In defense of the “tunneling” wave function of the universe
Open Access
- 15 August 1997
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 56 (4) , 2464-2468
- https://doi.org/10.1103/physrevd.56.2464
Abstract
The tunneling approach to the wave function of the Universe has been recently criticized by Bousso and Hawking who claim that it predicts a catastrophic instability of de Sitter space with respect to pair production of black holes. We show that this claim is unfounded. First, we argue that different horizon size regions in de Sitter space cannot be treated as independently created, as they contend. And second, the WKB tunneling wave function is not simply the “inverse” of the Hartle-Hawking one, except in very special cases. Applied to the related problem of pair production of massive particles, we argue that the tunneling wave function leads to a small constant production rate, and not to a catastrophe as the argument of Bousso and Hawking would suggest.Keywords
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This publication has 21 references indexed in Scilit:
- Pair creation of black holes during inflationPhysical Review D, 1996
- Cosmological production of charged black hole pairsPhysical Review D, 1995
- Stochastic approach to tunneling and baby universe formationNuclear Physics B, 1992
- Black holes and quantum wormholesPhysics Letters B, 1989
- Boundary conditions in quantum cosmologyPhysical Review D, 1986
- Quantum mechanics in the tunneling universePhysics Letters B, 1984
- Quantum creation of universesPhysical Review D, 1984
- The quantum state of the universeNuclear Physics B, 1984
- Wave function of the UniversePhysical Review D, 1983
- Semiclassical perdurance of de Sitter spaceNuclear Physics B, 1983