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- W2800698865 abstract "We consider a vacuum static spacetime in a finite size cavity. On the boundary, we specify a metric and a finite constant local temperature [Formula: see text]. No spherical or any other spatial symmetry is assumed. We show that (i) inside a cavity, only a black hole or flat spacetime are possible, whereas a curved horizonless regular spacetime is excluded, (ii) in the limit when the horizon area shrinks, the Hawking temperature diverges, (iii) for the existence of a black hole, [Formula: see text] should be high enough. When [Formula: see text], a black hole phase is favorable thermodynamically. Our consideration essentially uses the coordinate system introduced by Israel in his famous proof of the uniqueness theorem." @default.
- W2800698865 created "2018-05-17" @default.
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- W2800698865 date "2019-03-12" @default.
- W2800698865 modified "2023-09-26" @default.
- W2800698865 title "Distorted vacuum black holes in the canonical ensemble" @default.
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- W2800698865 doi "https://doi.org/10.1142/s0217732319500603" @default.
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