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Black hole mass spectrum vs spectrum of Hawking radiation
General Relativity and Quantum Cosmology · Submitted 10 Aug 1998
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim It means that the structure of black hole is changing during its evaporation resulting in the Bekenstein-Mukhanov spectrum for large masses.
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The abstract, sentence by sentence
We consider a massive selfgravitating shell as a model for collapsing body and a null selfgravitating shell as a model for quanta of Hawking radiation. It is show that the mass-energy spectra for the body and the radiation do not match. The way out of this difficulty is to consider not only out-going radiation but also the ingoing one. It means that the structure of black hole is changing during its evaporation resulting in the Bekenstein-Mukhanov spectrum for large masses.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We consider a massive selfgravitating shell as a model for collapsing body and a null selfgravitating shell as a model for quanta of Hawking radiation. | method 0.95 | 0.58 | 0.03 | asserted 0.88 |
| s1 | It is show that the mass-energy spectra for the body and the radiation do not match. | result 0.98 | 0.80 | 0.48 | asserted 1.00 |
| s2 | The way out of this difficulty is to consider not only out-going radiation but also the ingoing one. | contribution 0.45 | 0.42 | 0.12 | asserted 0.79 |
| s3 | It means that the structure of black hole is changing during its evaporation resulting in the Bekenstein-Mukhanov spectrum for large masses. | interpretation 0.89 | 0.67 | 0.67 | asserted 0.96 |
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The paper
Original abstract
We consider a massive selfgravitating shell as a model for collapsing body and a null selfgravitating shell as a model for quanta of Hawking radiation. It is show that the mass-energy spectra for the body and the radiation do not match. The way out of this difficulty is to consider not only out-going radiation but also the ingoing one. It means that the structure of black hole is changing during its evaporation resulting in the Bekenstein-Mukhanov spectrum for large masses.
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This property is in contrast with several other investigations of black hole spectra [ref] where a discrete spectrum is postulated or obtained [ref] .
Group quantization of the black hole minisuperspace · Mass operator · 0.95
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