The black hole final state for the Dirac fields in Schwarzschild spacetime

被引：53

作者：

Ahn, D. ^{[1
]}

Moon, Y. H. ^{[1
]}

Mann, R. B. ^{[2
]}

Fuentes-Schuller, I. ^{[3
]}

机构：

[1] Univ Seoul, Inst Quantum Informat Proc & Syst, Seoul 130743, South Korea

[2] Univ Waterloo, Dept Phys, Waterloo, ON N2L 3G1, Canada

[3] Univ Potsdam, Inst Phys, D-14469 Potsdam, Germany

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2008年 / 06期

关键词：

black holes in string theory; black holes;

D O I：

10.1088/1126-6708/2008/06/062

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We show that the internal stationary state of a black hole for massless Dirac fields can be represented by an entangled state of collapsing matter and infalling Hawking radiation. This implies that the Horowitz-Maldacena conjecture for the black hole final state originally proposed for the massless scalar fields is also applicable to fermionic fields as well. For an initially mixed state we find that the measure of mixedness is expected to decrease under evaporation.

引用

页数：10

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