CENTRIFUGAL FORCE IN KERR GEOMETRY

被引：17

作者：

IYER, S

PRASANNA, AR

机构：

[1] Physical Research Laboratory

来源：

CLASSICAL AND QUANTUM GRAVITY | 1993年 / 10卷 / 01期

关键词：

D O I：

10.1088/0264-9381/10/1/003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the 3 + 1 splitting of optical reference geometry, we have obtained the correct expression for the centrifugal force acting on a particle at the equatorial circumference of a rotating body in the locally non-rotating frame of the Kerr geometry. In contrast to the analysis based on Boyer-Lindquist coordinates, this expression is valid everywhere outside the event horizon.

引用

页码：L13 / L16

页数：4

共 5 条

[1]

ABRAMOWICZ MA, 1990, MON NOT R ASTRON SOC, V245, P729

[2]

ABRAMOWICZ MA, 1990, MON NOT R ASTRON SOC, V245, P720

[3] OPTICAL REFERENCE GEOMETRY FOR STATIONARY AND STATIC DYNAMICS [J].