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- W2089979197 abstract "We trace the origin of the black hole entropy S by replacing a black hole by a quasiblack hole. Let the boundary of a static body approach its own gravitational radius, in such a way that a quasihorizon forms. We show that if the body is thermal with the temperature taking the Hawking value at the quasihorizon limit, it follows, in the nonextremal case, from the first law of thermodynamics that the entropy approaches the Bekenstein-Hawking value S = A/4. The entropy comes from the quasihorizon surface. For extremal quasiblack holes, the entropy S is model-dependent and depends also on the way the temperature at infinity approaches zero value." @default.
- W2089979197 created "2016-06-24" @default.
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- W2089979197 date "2011-01-01" @default.
- W2089979197 modified "2023-09-25" @default.
- W2089979197 title "QUASIBLACK HOLES AND BLACK HOLE ENTROPY" @default.
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- W2089979197 doi "https://doi.org/10.1142/s2010194511001486" @default.
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