2001
DOI: 10.1023/a:1012930019453
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Cited by 32 publications
(28 citation statements)
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“…Trans-Hawking versions of Hawking radiation, either as reformulations of the physics, or as alternative scenarios [62, 120, 222, 223, 257, 266, 278, 279, 280, 384, 478, 480, 530, 536, 541, 542, 549, 550, 567, 591]. …”
Section: Phenomenology Of Analogue Modelsmentioning
confidence: 99%
“…Trans-Hawking versions of Hawking radiation, either as reformulations of the physics, or as alternative scenarios [62, 120, 222, 223, 257, 266, 278, 279, 280, 384, 478, 480, 530, 536, 541, 542, 549, 550, 567, 591]. …”
Section: Phenomenology Of Analogue Modelsmentioning
confidence: 99%
“…Trans-Hawking versions of Hawking radiation, either as reformulations of the physics, or as alternative scenarios [30, 68, 130, 131, 150, 156, 167, 168, 169, 233, 289, 291, 325, 329, 333, 334, 340, 341, 350, 364]. …”
Section: Lessons From Analogue Modelsmentioning
confidence: 99%
“…Instead, it has the maximum value at this point and becomes zero at M = M IR1 . In order to study the phase transition explicitly, let us introduce the off-shell free energy, which plays a role of effective potential in the canonical ensemble, as follows [12,17,19,20]:…”
Section: Ir System: Schwarzschild Black Hole In a Cavitymentioning
confidence: 99%
“…We call the phase transition between thermal radiation and the large black hole in a cavity as the well-defined Gross-Perry-Yaffe (WGPY) transition 1 . The WGPY transition could be checked by observing the heat capacity and free energy [17]. Our work is based on the first law of dE = T dS rather than dM = T dS.…”
Section: Introductionmentioning
confidence: 99%