Renyi entropies of a black hole from Hawking radiation

被引:30
作者
Bialas, A. [1 ]
Czyz, W.
机构
[1] Jagellonian Univ, M Smoluchowski Inst Phys, PL-30059 Krakow, Poland
关键词
D O I
10.1209/0295-5075/83/60009
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Renyi entropies of a black hole are evaluated by counting the states of the Hawking radiation which fills a thin shell surrounding the horizon. The width of the shell is determined from its energy content and the corresponding mass defect. The Bekenstein-Hawking formula for the entropy of the black hole is correctly reproduced. Copyright c (c) EPLA, 2008
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页数:3
相关论文
共 9 条
[1]   GENERALIZED SECOND LAW OF THERMODYNAMICS IN BLACK-HOLE PHYSICS [J].
BEKENSTE.JD .
PHYSICAL REVIEW D, 1974, 9 (12) :3292-3300
[2]  
Bialas A, 2000, ACTA PHYS POL B, V31, P2803
[3]   BREAKDOWN OF PREDICTABILITY IN GRAVITATIONAL COLLAPSE [J].
HAWKING, SW .
PHYSICAL REVIEW D, 1976, 14 (10) :2460-2473
[4]   BLACK-HOLES AND THERMODYNAMICS [J].
HAWKING, SW .
PHYSICAL REVIEW D, 1976, 13 (02) :191-197
[5]  
Landau L. D., 1975, The Classical Theory of Fields
[6]  
Landau L. D., 2013, Statistical Physics
[7]  
Renyi A., 1961, P 4 BERKELEY S MATH, V1, P547
[8]   The paradox of quantum black holes [J].
Susskind, Leonard .
NATURE PHYSICS, 2006, 2 (10) :665-677
[9]   ON THE QUANTUM STRUCTURE OF A BLACK-HOLE [J].
THOOFT, G .
NUCLEAR PHYSICS B, 1985, 256 (04) :727-745