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.
|Titolo:||Fast and Accurate Computation of Gravitational Waveforms from Binary Stars with any Orbital Eccentricity|
|Data di pubblicazione:||2001|
|Appare nelle tipologie:||1.1 Articolo in rivista|