Abstract
The Hawking temperature of a Schwarzschild black hole can be heuristically derived by identifying the temperature with the inverse radius of the horizon up to a multiplicative constant. This does not work for more general black holes such as the Kerr and Reissner–Nordström solutions. Expounding on the details of how it fails to work nevertheless uncovers some connections with the “spring constant” of black holes and with black hole thermodynamics.
Original language | English |
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Article number | 169919 |
Journal | Annals of Physics |
Volume | 474 |
DOIs | |
Publication status | Published - Mar 2025 |
Keywords
- Black hole thermodynamics
- Hawking radiation
- Surface gravity
ASJC Scopus subject areas
- General Physics and Astronomy