Evaporation of Schwarzschild black holes in Matrix Theory

被引：24

作者：

Banks, T

Fischler, W

Klebanov, IR

机构：

[1] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08855 USA

[2] Univ Texas, Dept Phys, Theory Grp, Austin, TX 78712 USA

[3] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA

来源：

PHYSICS LETTERS B | 1998年 / 423卷 / 1-2期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0370-2693(98)00118-X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Recently, in collaboration with Susskind, we proposed a model of Schwarzschild black holes in Matrix Theory. A large Schwarzschild black hole is described by a metastable bound state of a large number of D0-branes which are held together by a background, whose structure has so far been understood only in 8 and Il dimensions. The Hawking radiation proceeds by emission of small clusters of D0-branes. We estimate the Hawking rate in the Matrix Theory model of Schwarzschild black holes and find agreement with the semiclassical rate up to an undetermined numerical coefficient of order 1. (C) 1998 Published by Elsevier science B.V.

引用

页码：54 / 58

页数：5

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