Published March 15, 1999 | Version Published
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Mapping Hawking into Unruh thermal properties

  • 1. ROR icon Brandeis University

Abstract

By globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal properties map into their Unruh equivalents: The relevant curved space detectors become Rindler ones, whose temperature and entropy reproduce the originals. Specific illustrations include Schwarzschild, Schwarzschild–(anti-)de Sitter, Reissner-Nordström, and Bañados-Teitelboim-Zanelli spaces.

Additional Information

© 1999 American Physical Society. (Received 22 October 1998; published 1 February 1999) We thank M. Banados for useful discussions of BTZ. This work was supported by NSF grant PHY-9315811 and by the Fishbach Foundation for OL.

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Identifiers

Eprint ID
73378
Resolver ID
CaltechAUTHORS:20170110-122327553

Related works

Funding

NSF
PHY-9315811
Fishbach Foundation

Dates

Created
2017-01-10
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Updated
2021-11-11
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