Hawking temperature and the inverse-radius scale of the horizon

Michael R.R. Good, Yen Chin Ong

Research output: Contribution to journalArticlepeer-review

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 languageEnglish
Article number169919
JournalAnnals of Physics
Volume474
DOIs
Publication statusPublished - Mar 2025

Keywords

  • Black hole thermodynamics
  • Hawking radiation
  • Surface gravity

ASJC Scopus subject areas

  • General Physics and Astronomy

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