Information recovery from black holes

被引:14
作者
Balasubramanian, Vijay [1 ]
Marolf, Donald
Rozali, Moshe
机构
[1] Univ Penn, David Rittenhouse Labs, Philadelphia, PA 19104 USA
[2] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[3] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[4] Perimeter Inst, Waterloo, ON N2L 2Y5, Canada
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2006年 / 15卷 / 12期
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词
black holes; black hole information;
D O I
10.1142/S0218271806009765
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We argue that if black hole entropy arises from a finite number of underlying quantum states, then any particular such state can be identified from infinity. The finite density of states implies a discrete energy spectrum, and, in general, such spectra are non-degenerate except as determined by symmetries. Therefore, knowledge of the precise energy, and of other commuting conserved charges, determines the quantum state. In a gravitating theory, all conserved charges including the energy are given by boundary terms that can be measured at infinity. Thus, within any theory of quantum gravity, no information can be lost in black holes with a finite number of states. However, identifying the state of a black hole from infinity requires measurements with Planck scale precision. Hence, observers with insufficient resolution will experience information loss.
引用
收藏
页码:2285 / 2292
页数:8
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