Excitation of the odd parity quasinormal modes of compact objects

被引：23

作者：

Andrade, Z ^{[1
]}

Price, RH ^{[1
]}

机构：

[1] Univ Utah, Dept Phys, Salt Lake City, UT 84112 USA

来源：

PHYSICAL REVIEW D | 1999年 / 60卷 / 10期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevD.60.104037

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The gravitational radiation generated by a particle in a close unbounded orbit around a neutron star is computed as a means to study the importance of the w modes of the neutron star. For simplicity, attention is restricted to odd parity ("axial") modes which do not couple to the neutron star's fluid modes. We find that for realistic neutron star models, particles in unbounded orbits only weakly excite the w modes; we conjecture that this is also the case For astrophysically interesting sources of neutron star perturbations. We also find that for cases in which there is significant excitation of quadrupole w modes, there is comparable excitation of higher multipole modes. [S0556-2821(99)03822-9].

引用

页数：3

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