Radiation equations for black holes

被引：10

作者：

Vilkovisky, GA

机构：

[1] Lebedev Phys Inst, Moscow 119991, Russia

[2] Lebedev Res Ctr Phys, Moscow 119991, Russia

来源：

PHYSICS LETTERS B | 2006年 / 634卷 / 5-6期

关键词：

D O I：

10.1016/j.physletb.2006.02.012

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It has been shown in [G.A. Vilkovisky, hep-th/0511182] that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the Bondi charges are expressed through this metric by calculating the vacuum radiation against its background. The result is closed equations for the metric and the Bondi charges. Notably, there is a nonvanishing flux of the vacuum-induced matter charge. (c) 2006 Elsevier B.V. All rights reserved.

引用

页码：456 / 464

页数：9

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