THE ENERGY-MOMENTUM TENSOR OF A BLACK-HOLE, OR WHAT CURVES THE SCHWARZSCHILD GEOMETRY

被引：61

作者：

BALASIN, H

NACHBAGAUER, H

机构：

[1] Inst. fur Theor. Phys., Tech. Wien Univ.

来源：

CLASSICAL AND QUANTUM GRAVITY | 1993年 / 10卷 / 11期

关键词：

D O I：

10.1088/0264-9381/10/11/010

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using distributional techniques we calculate the energy-momentum tensor of the Schwarzschild geometry. It turns out to be a well defined tensor distribution concentrated on the r = 0 region which is usually excluded from spacetime. This provides a physical interpretation for the curvature of this geometry.

引用

页码：2271 / 2278

页数：8

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[No title captured]

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