Abstract
Starting from the Einstein-Boltzmann formula we determine classically the second moments for the fluctuations of a massive Schwarzschild black hole enclosed with thermal radiation in a rigid box. © 1983.
Original language | English |
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Pages (from-to) | 214-216 |
Journal | Physics Letters A |
Volume | 99 |
Issue number | 5 |
DOIs | |
Publication status | Published - 5 Dec 1983 |