Information recovery from black holes

被引:30
|
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
关键词
black holes; black hole information;
D O I
10.1007/s10714-006-0344-8
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:1529 / 1536
页数:8
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