Tunneling during Quantum Collapse in AdS Spacetime

Abstract

We extend previous results on the reflection and transmission of self-gravitating dust shells across the apparent horizon during quantum dust collapse to non-marginally-bound dust collapse in arbitrary dimensions with a negative cosmological constant. We show that the Hawking temperature is independent of the energy function and that the wave functional describing the collapse is well behaved at the Hawking-Page transition point. Thermal radiation from the apparent horizon appears as a generic result of non-marginal collapse in AdS space-time owing to the singular structure of the Hamiltonian constraint at the apparent horizon.

14 pages. No figures. Title changed to published version

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Cited by in corpus (5)

• Black Holes: Eliminating Information or Illuminating New Physics?
• Black holes as Gravitational Atoms
• Quantum gravitational dust collapse does not result in a black hole
• Infrared signatures of quantum bounce in a minisuperspace analysis of Lema\^ıtre-Tolman-Bondi dust collapse
• A quantum thin shell surrounding a Black Hole