Gravitational waves from the pulsar magnetosphere

被引：1
|
作者：
Contopoulos, Ioannis [1 ]
Kazanas, Demosthenes [2 ]
Papadopoulos, Demetrios B. [3 ]
机构：
[1] Acad Athens, Res Ctr Astron & Appl Math, 4 Soranou Efessiou Str, Athens 11527, Greece
[2] Goddard Space Flight Ctr, NASA, Astrophys Sci Div, Greenbelt, MD 20771 USA
[3] Aristotle Univ Thessaloniki, Dept Phys, Sect Astrophys Astron & Theoret Mech, Saloniki 54124, Greece
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2024年 / 527卷 / 04期
关键词：
gravitational waves; MHD; pulsars: general; ELECTRODYNAMICS;
D O I：
10.1093/mnras/stad3913
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We investigate the generation of gravitational waves from the rotation of an orthogonal pulsar magnetosphere in flat space-time. We calculate the first-order metric perturbation due to the rotation of the non-axisymmetric distribution of electromagnetic energy density around the central star. We show that gravitational waves from a strong magnetic field pulsar right after its formation within a distance of 1 kpc may be detectable with the new generation of gravitational wave detectors.
引用
收藏
页码：11198 / 11205
页数：8
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