Quantum Black Holes from Quantum Collapse
arXiv:gr-qc/0104017 · doi:10.1103/PhysRevD.64.084005
Abstract
The Schwarzschild black hole can be viewed as the special case of the marginally bound Lema\^ıtre-Tolman-Bondi models of dust collapse which corresponds to a constant mass function. We have presented a midi-superspace quantization of this model for an arbitrary mass-function in a separate publication. In this communication we show that our solution leads both to Bekenstein's area spectrum for black holes as well as to the black hole entropy, which, in this context, is naturally interpreted as the loss of information of the original matter distribution within the collapsing dust cloud.
LaTeX file, 6 pages, 1 figure, Paper re-written into sections, some references added, some elaborations, conclusions unchanged, to appear in Physical Review D
References in corpus (1)
Cited by in corpus (23)
- Quantum tunneling and black hole spectroscopy
- Singularity avoidance for collapsing quantum dust in the Lemaitre-Tolman-Bondi model
- Classical and quantum LTB model for the non-marginal case
- Quantization of Midisuperspace Models
- Hawking radiation from the quantum Lemaitre-Tolman-Bondi model
- Mass Spectrum and Statistical Entropy of the BTZ black hole from Canonical Quantum Gravity
- Building blocks of a black hole
- Gibbs' paradox and black-hole entropy
- Quantum general relativity and Hawking radiation
- Exact Quantum State of Collapse and Black Hole Radiation
- Canonical Quantization of Spherically Symmetric Dust Collapse
- Spectrum of quantized black hole, correspondence principle, and holographic bound
- Quantized Black Holes, Their Spectrum and Radiation
- How Is the Maximum Entropy of a Quantized Surface Related to Its Area?
- Entropy and Area of Black Holes in Loop Quantum Gravity
- Reflection and Transmission at the Apparent Horizon during Gravitational Collapse
- Canonical Partition function of Loop Black Holes
- Infrared signatures of quantum bounce in a minisuperspace analysis of Lema\^ıtre-Tolman-Bondi dust collapse
- Self-gravitating stellar collapse: explicit geodesics and path integration
- Numerical thermodynamic studies of classical gravitational collapse in 3+1 and 4+1 dimensions
- Role of Gauss-Bonnet corrections in a DGP brane gravitational collapse
- Directly observing entropy accumulate on the horizon and holography
- Formation of a condensate during charged collapse