INTERACTION OF PRIMORDIAL GRAVITATIONAL WAVES WITH GROUPS OF GALAXIES

被引：1

作者：

REES, MJ

机构：

[1] Harvard College Observatory, Cambridge,MA,02138, United States

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1972年 / 159卷 / 03期

关键词：

Astrophysics - Galaxies - Gravitational effects - NASA;

D O I：

10.1093/mnras/159.1.11P

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Two processes whereby very long wavelength gravitational waves may cumulatively feed energy into a cluster of galaxies during its lifetime are considered, and found to be unimportant. The only potentially observable manifestation of primordial gravitational radiation is the velocity dispersion induced by waves currently interacting with groups of galaxies, as discussed in an earlier paper by the present author. © 1972 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.

引用

页码：P11 / &

共 5 条

[1] GRAVITATIONAL RADIATION IN LIMIT OF HIGH FREQUENCY .2. NONLINEAR TERMS AND EFFECTIVE STRESS TENSOR [J].