SUBTLETIES IN THE QUASI-CLASSICAL CALCULATION OF HAWKING RADIATION

被引：144

作者：

Akhmedov, Emil T. ^{[1
]}

Pilling, Terry ^{[2
]}

Singleton, Douglas ^{[3
]}

机构：

[1] ITEP, Moscow 117218, Russia

[2] N Dakota State Univ, Dept Phys, Fargo, ND 58105 USA

[3] Calif State Univ Fresno, Dept Phys, Fresno, CA 93740 USA

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2008年 / 17卷 / 13-14期

关键词：

D O I：

10.1142/S0218271808013947

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The quasi-classical method of deriving Hawking radiation is investigated. In order to recover the original Hawking temperature one must take into account a previously ignored contribution coming from the temporal part of the action. This contribution plus a contribution coming from the spatial part of the action gives the correct temperature.

引用

页码：2453 / 2458

页数：6

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