The scalar ether-theory of gravitation and its first test in celestial mechanics

被引:7
作者
Arminjon, M [1 ]
机构
[1] CNRS, Lab Sols Solides Struct, UMR 5521, F-38041 Grenoble 9, France
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2002年 / 17卷 / 29期
关键词
alternative theories; preferred frame; post-Newtonian; celestial mechanics;
D O I
10.1142/S0217751X0201323X
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The motivations for investigating a theory of gravitation based on a concept of "ether" are discussed - a crucial point is the existence of an alternative interpretation of special relativity, named the Lorentz-Poincare ether theory. The basic equations of one such theory of gravity, based on just one scalar field, axe presented. To check this theory in celestial mechanics, an "asymptotic" scheme of post-Newtonian (PN) approximation is summarized and. its difference with the standard PN scheme is emphasized. The derivation of PN equations of motion for the mass centers, based on the asymptotic scheme, is outlined. They are implemented for the major bodies of the solar system and the prediction for Mercury is compared with an ephemeris based on general relativity.
引用
收藏
页码:4203 / 4208
页数:6
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