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A complementary third law for black hole thermodynamics
Stockholm University, Nordic Institute for Theoretical Physics (Nordita). Yangzhou University, China; Shanghai Jiao Tong University, China.
Number of Authors: 32019 (English)In: European Physical Journal C, ISSN 1434-6044, E-ISSN 1434-6052, Vol. 79, no 6, article id 513Article in journal (Refereed) Published
Abstract [en]

There are some examples in the literature, in which despite the fact that the underlying theory or model does not impose a lower bound on the size of black holes, the final temperature under Hawking evaporation is nevertheless finite and nonzero. We show that under some loose conditions, the black hole is necessarily an effective remnant, in the sense that its evaporation time is infinite. That is, the final state that there is nonzero finite temperature despite having no black hole remaining cannot be realized. We discuss the limitations, subtleties, and the implications of this result, which is reminiscent of the third law of black hole thermodynamics, but with the roles of temperature and size interchanged. We therefore refer to our result as the complementary third law for black hole thermodynamics.

Place, publisher, year, edition, pages
2019. Vol. 79, no 6, article id 513
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-171130DOI: 10.1140/epjc/s10052-019-7003-1ISI: 000471628700002OAI: oai:DiVA.org:su-171130DiVA, id: diva2:1343574
Available from: 2019-08-17 Created: 2019-08-17 Last updated: 2019-08-17Bibliographically approved

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