Fast and Accurate Computation Tools for Gravitational Waveforms from Binary Sistems with any Orbital Eccentricity

TL;DR

This paper introduces efficient and precise computational tools for generating gravitational wave templates from binary systems with arbitrary orbital eccentricity, enhancing detection capabilities.

Contribution

It presents novel fast and accurate methods for modeling gravitational waveforms from eccentric binary systems, including error estimation techniques.

Findings

Tools enable rapid waveform computation for any eccentricity

Error bounds improve template accuracy

Enhances gravitational wave detection sensitivity

Abstract

The relevance of orbital eccentricity in the detection of gravitational radiation from (steady state) binary stars is emphasized. Computationnally 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.