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Most of compact binary systems are expected to circularize before the frequency of emitted gravitational waves (GWs) enters the sensitivity band of the ground based interferometric detectors.
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Search for Gravitational Waves from Low Mass Compact Binary Coalescence in 186 Days of LIGO’s fifth Science Run,
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Post-Circular Expansion of Eccentric Binary Inspirals: Fourier-Domain Waveforms in the Stationary Phase Approximation,
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Search for gravitational-wave bursts in the first year of the fifth LIGO science run,
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Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors,
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The effect of eccentricity on searches for gravitational-waves from coalescing compact binaries in ground-based detectors,
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LIGO S6 detector characterization studies,
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W. E. East, S.T. McWilliams, J. Levin, and F. Pretorius, · 2012
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Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010,
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Effect of eccentricity on binary neutron star searches in Advanced LIGO,
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Shattering flares during close encounters of neutron stars,
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Accurate and efficient waveforms for compact binaries on eccentric orbits,
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Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run,
LIGO-Virgo Collaboration, · 2014
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Detectability of eccentric compact binary coalescences with advanced gravitational-wave detectors,
M. Coughlin, P. Meyers, et al., · 2015
Closest in time.
Detection and reconstruction of gravitational wave transients with networks of advanced detectors,
S. Klimenko, G. Vedovato, et al., · 2015
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Reconstruction of Chirp Mass in the Search of Compact Binaries,
V. Tiwari, S. Klimenko, et al., · 2015
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