Upper bound on the energies of the emitted Hawking quanta
Using Thorne's hoop conjecture, it is argued that the energies of the Hawking quanta emitted from canonical Schwarzschild black holes are bounded from above by the simple quantum relation E<Emax=ħ2/3/M1/3. In particular, it is shown that, due to non-linear (self-gravity) effects of the tunne...
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| Format: | Article |
| Language: | English |
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Elsevier
2019-05-01
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| Series: | Nuclear Physics B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0550321319300719 |