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- W3098047666 abstract "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." @default.
- W3098047666 created "2020-11-23" @default.
- W3098047666 creator A5063240935 @default.
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- W3098047666 date "2019-06-01" @default.
- W3098047666 modified "2023-10-12" @default.
- W3098047666 title "A complementary third law for black hole thermodynamics" @default.
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- W3098047666 doi "https://doi.org/10.1140/epjc/s10052-019-7003-1" @default.
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