ENTROPY, AREA, AND BLACK-HOLE PAIRS

被引:387
作者
HAWKING, SW [1 ]
HOROWITZ, GT [1 ]
ROSS, SF [1 ]
机构
[1] UNIV CAMBRIDGE,ISAAC NEWTON INST MATH SCI,CAMBRIDGE CB3 0EH,ENGLAND
来源
PHYSICAL REVIEW D | 1995年 / 51卷 / 08期
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevD.51.4302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We clarify the relation between gravitational entropy and the area of horizons. We first show that the entropy of an extreme Reissner-Nordström black hole is zero, despite the fact that its horizon has nonzero area. Next, we consider the pair creation of extremal and nonextremal black holes. It is shown that the action which governs the rate of this pair creation is directly related to the area of the acceleration horizon and (in the nonextremal case) the area of the black hole event horizon. This provides a simple explanation of the result that the rate of pair creation of nonextreme black holes is enhanced by precisely the black hole entropy. Finally, we discuss black hole annihilation, and argue that Planck scale remnants are not sufficient to preserve unitarity in quantum gravity. © 1995 The American Physical Society.
引用
收藏
页码:4302 / 4314
页数:13
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