THE ULTRARELATIVISTIC KERR GEOMETRY AND ITS ENERGY-MOMENTUM TENSOR

被引：58

作者：

BALASIN, H

NACHBAGAUER, H

机构：

[1] ENSLAPP, PHYS THEOR LAB, CNRS, URA 1436, F-74941 ANNECY LE VIEUX, FRANCE

[2] ENSLAPP, PHYS THEOR LAB, IN2P3, CNRS, F-74941 ANNECY LE VIEUX, FRANCE

来源：

CLASSICAL AND QUANTUM GRAVITY | 1995年 / 12卷 / 03期

关键词：

D O I：

10.1088/0264-9381/12/3/009

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ultrarelativistic limit of the Schwarzschild and Kerr geometries, together with their respective energy-momentum tensors, is derived. Our approach is based on tenser distributions making use of the underlying Kerr-Schild structure, which remains stable under the ultrarelativistic boost.

引用

页码：707 / 713

页数：7

共 9 条

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