Fast and accurate computational tools for gravitational waveforms from binary stars with any orbital eccentricity

被引：37

作者：

Pierro, V ^{[1
]}

Pinto, IM

Spallicci, AD

Laserra, E

Recano, F

机构：

[1] Univ Sannio Benevento, Waves Grp, Salerno, Italy

[2] Univ Salerno, IMA, I-84100 Salerno, Italy

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2001年 / 325卷 / 01期

关键词：

gravitational waves; methods : data analysis; binaries : general;

D O I：

10.1046/j.1365-8711.2001.04442.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The relevance of orbital eccentricity in the detection of gravitational radiation from (steady state) binary stars is emphasized. Computationally effective (fast and accurate) tools for constructing gravitational wave templates from binary stars with any orbital eccentricity are introduced including tight estimation criteria of the pertinent truncation and approximation errors.

引用

页码：358 / 372

页数：15

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