Orbital dynamics of extreme charged black hole

被引：18

作者：

Chen, JH ^{[1
]}

Wang, YJ ^{[1
]}

机构：

[1] Hunan Normal Univ, Inst Phys, Dept Phys, Changsha 410081, Peoples R China

来源：

ACTA PHYSICA SINICA | 2001年 / 50卷 / 10期

关键词：

phase-plane; stability; orbit;

D O I：

10.7498/aps.50.1833

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

With the phase-plane analysis method, we obtain the general relativity motion equation in the gravitational field of the extreme charged black hole, and we plot the picture of the orbital phase-plane and analyze the orbital stability.

引用

页码：1833 / 1836

页数：4

共 14 条

[1]

ARYA AP, 1990, INTRO CLASSICAL MECH, P222

[2]

CORBEN HC, 1994, CLASSICAL MECH, P90

[3] ELEMENTARY THEORY OF PERIHELION PRECESSION [J].

DAVIES, B .

AMERICAN JOURNAL OF PHYSICS, 1983, 51 (10) :909-911

[4]

DAVIES B, 1988, AM J PHYS, V56, P1097

[5]

DAVIES B, 1985, AM J PHYS, V53, P374

[6]

FOWLES G, 1993, CLASSICAL DYNAMICS P, P191

[7]

GOLDSTEIN H, 1980, CLASSICAL MECH, P94

[8]

KOMPANEYETS AS, 1962, THEORETICAL MECH, P41

[9]

MARION J, 1995, ANAL MECH, P291

[10]

MARTIN JL, 1996, GEN RELATIVITY FIRST, P58

← 1 2 →