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

2000/05/12 by V. Pierro, I. M. Pinto, A. Spallicci +4 · 3 citations
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #Geophysics and Gravity Measurements #Pulsars and Gravitational Waves Research #gr-qc

paper · pdf · doi:10.1046/j.1365-8711.2001.04442.x

published as Mon.Not.Roy.Astron.Soc. 325 (2001) 358 · submitted to Mon. Not. Roy. Astron. Soc., under review. 11 Pages, 45 Figures

arxiv created 2000/05/12 · openalex publication_date 2001/07/11 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

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.

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