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arXiv · gr-qc/9908043

Detection of Gravitational Waves from Eccentric Compact Binaries

Karl Martel
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Abstract

Coalescing compact binaries have been pointed out as the most promising source of gravitational waves for kilometer-size interferometers such as LIGO. Gravitational wave signals are extracted from the noise in the detectors by matched filtering. This technique performs really well if an a priori theoretical knowledge of the signal is available. The information known about the possible sources is used to construct a model of the expected waveforms (templates). A common assumption made when constructing templates for coalescing compact binaries is that the companions move in a quasi-circular orbit. Some scenarios, however, predict the existence of eccentric binaries. We investigate the loss in signal-to-noise ratio induced by non-optimal filtering of eccentric signals.

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Karl Martel. 1999-08-13. Detection of Gravitational Waves from Eccentric Compact Binaries. https://doi.org/10.1063/1.1301562

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