Gravitational wave emission from galactic radio pulsars

被引：4

作者：

Pacheco, JAD ^{[1
]}

Horvath, JE ^{[1
]}

机构：

[1] UNIV SAO PAULO,INST ASTRON & GEOFIS,BR-04302904 SAO PAULO,BRAZIL

来源：

PHYSICAL REVIEW D | 1997年 / 56卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.56.859

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We consider in this work continuous gravitational wave (GW) emission from nonaxisymmetric radio pulsars. We treat in some detail the observational issues related to the known radio pulsar sample with the aim of unveiling the actual number of sources contributing to GW, which are likely to be the main contributors of GW's. It is shown that the operation of spheroidal GW detectors and full-size interferometers could detect this component of the radiation or impose useful limits on the effective oblateness of young radio pulsars.

引用

页码：859 / 863

页数：5