QUASI-LOCAL MOMENTUM AND ANGULAR-MOMENTUM IN KERR SPACETIME

被引：14

作者：

BERGQVIST, G ^{[1
]}

LUDVIGSEN, M ^{[1
]}

机构：

[1] LINKOPING UNIV,DEPT MATH,S-58183 LINKOPING,SWEDEN

来源：

CLASSICAL AND QUANTUM GRAVITY | 1991年 / 8卷 / 04期

关键词：

D O I：

10.1088/0264-9381/8/4/014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It is shown that the Kerr spacetime possesses a vector space V and an affine space M0 allowing definitions of quasilocal momentum and angular momentum with all the desired properties. The construction of V and M0 makes use of a natural, flat, metric connection with torsion and of a generalized twistor equation. The momentum and angular momentum contained within a finite 2-surface SIGMA are expressed as the integrals over SIGMA of two closed 2-forms.

引用

页码：697 / 701

页数：5

共 6 条

[1] SPINOR PROPAGATION AND QUASILOCAL MOMENTUM FOR THE KERR SOLUTION [J].