POINCARE GAUGE-THEORY OF GRAVITATION AND THE BINARY PULSAR 1913 + 16

被引：31

作者：

SCHWEIZER, M

STRAUMANN, N

机构：

[1] Institute for Theoretical Physics, the University of Zürich

来源：

PHYSICS LETTERS A | 1979年 / 71卷 / 5-6期

关键词：

D O I：

10.1016/0375-9601(79)90645-5

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The post-newtonian approximations of a Poincaré gauge theory of gravitation, recently proposed by Hehl et al., are shown to agree with Einstein's theory to fourth order. In addition, Einstein's quadrupole formula for the gravitational radiation holds in a naive linearized approximation. Hence, the theory is not only in agreement with solar system tests, but is also consistent with recent observations of the binary pulsar 1913 + 16. © 1979.

引用

页码：493 / 495

页数：3

共 7 条

[1] SHORT-RANGE CONFINING COMPONENT IN A QUADRATIC POINCARE GAUGE THEORY OF GRAVITATION [J].