A CLASSICAL INSTABILITY OF REISSNER-NORDSTROM SOLUTIONS AND THE FATE OF MAGNETICALLY CHARGED BLACK-HOLES

被引：115

作者：

LEE, KY ^{[1
]}

NAIR, VP ^{[1
]}

WEINBERG, EJ ^{[1
]}

机构：

[1] FERMI NATL ACCELERATOR LAB,NASA,FERMILAB ASTROPHYS CTR,BATAVIA,IL 60510

来源：

PHYSICAL REVIEW LETTERS | 1992年 / 68卷 / 08期

关键词：

D O I：

10.1103/PhysRevLett.68.1100

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Working in the context of spontaneously broken gauge theories, we show that the magnetically charged Reissner-Nordstrom solution develops a classical instability if the horizon is sufficiently small. This instability has significant implications for the evolution of a magnetically charged black hole. In particular, it leads to the possibility that such a hole could evaporate completely, leaving in its place a nonsingular magnetic monopole.

引用

页码：1100 / 1103

页数：4