Hawking radiation as tunneling for extremal and rotating black holes

被引：351

作者：

Angheben, M ^{[1
]}

Nadalini, M

Vanzo, L

Zerbini, S

机构：

[1] Univ Trent, Dipartimento Fis, I-38050 Trento, Italy

[2] Ist Nazl Fis Nucl, Grp Coll Trent, I-38050 Trento, Italy

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2005年 / 05期

关键词：

space-time symmetries; black holes;

D O I：

10.1088/1126-6708/2005/05/014

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：

The issue concerning semi-classical methods recently developed in deriving the conditions for Hawking radiation as tunneling, is revisited and applied also to rotating black hole solutions as well as to the extremal cases. It is noticed how the tunneling method fixes the temperature of extremal black hole to be zero, unlike the euclidean regularity method that allows an arbitrary compactification period. A comparison with other approaches is presented.

引用

页码：274 / 291

页数：18

共 52 条

[1] Is the semi-classical analysis valid for extreme black holes? [J].