A heuristic way of obtaining the Kerr metric

被引:5
作者
Enderlein, J
机构
[1] CST-1, MS M888, Los Alamos National Laboratory, Los Alamos
关键词
D O I
10.1119/1.18679
中图分类号
G40 [教育学];
学科分类号
040101 ; 120403 ;
摘要
An intuitive, straightforward way of finding the metric of a rotating black hole is presented, based on the algebra of differential forms. The representation obtained for the metric displays a simplicity which is not obvious in the usual Boyer-Lindquist coordinates. (C) 1997 American Association of Physics Teachers.
引用
收藏
页码:897 / 902
页数:6
相关论文
共 6 条
[1]  
Chandrasekhar S, 1983, MATH THEORY BLACK HO, P273
[3]  
KRAMER D, 1981, EXACT SOLUTIONS EINS
[4]  
MARGENAU H, 1956, MATH PHYSICS CHEM, P182
[5]  
MISNER CW, 1973, GRAVITATION, P354
[6]  
Penrose R., 1984, SPINORS SPACE TIME, V1