Full asymptotic expansion of the relativistic orbit of a rest particle under the exact Schwarzschild metric

被引:8
作者
Do-Nhat, T [1 ]
机构
[1] Univ Waterloo, Dept Elect & Comp Engn, Waterloo, ON N2L 3G1, Canada
关键词
D O I
10.1016/S0375-9601(97)00883-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The perturbation method of Lindstedt and Poincare has been used for the derivation of the asymptotic expression of the relativistic orbit of a test particle influenced by the exact Schwarzschild metric, from which the perihelion advance of a test particle is expressed as a rapidly convergent power series. Numerical results show the convergence characteristics of the modified Newtonian orbital expression. (C) 1998 Elsevier Science B.V.
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页码:328 / 336
页数:9
相关论文
共 24 条
[1]  
Adler R., 1975, Introduction to General Relativity
[2]  
[Anonymous], 1953, The Meaning of Relativity
[3]  
BRUMBERG VA, 1991, Essential Relativistic Celestial Mechanics
[4]   HIGHER-ORDER RELATIVISTIC PERIASTRON ADVANCES AND BINARY PULSARS [J].
DAMOUR, T ;
SCHAFER, G .
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS, 1988, 101 (02) :127-176
[6]   RELATIVITY EFFECTS FOR THE 3 INNER PLANETS [J].
DUNCOMBE, RL .
ASTRONOMICAL JOURNAL, 1956, 61 (04) :174-175
[7]  
Einstein A, 1915, SITZBER K PREUSS AKA, P831
[8]  
HAGIWARA Y, 1977, ASTRONOMY, P30
[9]   QUADRUPOLE EFFECTS ON PLANETARY ORBITS [J].
HOENSELAERS, C .
PROGRESS OF THEORETICAL PHYSICS, 1976, 56 (01) :324-326
[10]   DISCOVERY OF A PULSAR IN A BINARY-SYSTEM [J].
HULSE, RA ;
TAYLOR, JH .
ASTROPHYSICAL JOURNAL, 1975, 195 (02) :L51-L53