SEMICLASSICAL STABILITY OF THE EXTREME REISSNER-NORDSTROM BLACK-HOLE

被引：75

作者：

ANDERSON, PR ^{[1
]}

HISCOCK, WA ^{[1
]}

LORANZ, DJ ^{[1
]}

机构：

[1] MONTANA STATE UNIV,DEPT PHYS,BOZEMAN,MT 59717

来源：

PHYSICAL REVIEW LETTERS | 1995年 / 74卷 / 22期

关键词：

D O I：

10.1103/PhysRevLett.74.4365

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The stress-energy tensor of a free quantized scalar field is calculated in the extreme Reissner-Nordström black hole spacetime in the zero-temperature vacuum state. The stress-energy appears to be regular on the event horizon, contrary to the suggestion provided by two-dimensional calculations. An analytic calculation on the event horizon for a thermal state shows that if the temperature is nonzero then the stress-energy diverges strongly there. © 1995 The American Physical Society.

引用

页码：4365 / 4368

页数：4

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