DISTRIBUTIONAL ENERGY-MOMENTUM TENSOR OF THE KERR-NEWMAN SPACETIME FAMILY

被引：55

作者：

BALASIN, H ^{[1
]}

NACHBAGAUER, H ^{[1
]}

机构：

[1] ENSLAPP,PHYS THEOR LAB,F-74941 ANNECY LE VIEUX,FRANCE

来源：

CLASSICAL AND QUANTUM GRAVITY | 1994年 / 11卷 / 06期

关键词：

D O I：

10.1088/0264-9381/11/6/010

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the Kerr-Schild decomposition of the metric tensor that employs the algebraically special nature of the Kerr-Newman spacetime family, we calculate the energy-momentum tensor. The latter turns out to be a well defined tensor distribution with disc-like support.

引用

页码：1453 / 1461

页数：9

共 13 条

[1] THE ENERGY-MOMENTUM TENSOR OF A BLACK-HOLE, OR WHAT CURVES THE SCHWARZSCHILD GEOMETRY [J].