TY - JOUR
T1 - Detecting gravitational waves from highly eccentric compact binaries
AU - Tai, Kai Sheng
AU - McWilliams, Sean T.
AU - Pretorius, Frans
N1 - Publisher Copyright:
© 2014 American Physical Society.
PY - 2014/11/10
Y1 - 2014/11/10
N2 - In dense stellar regions, highly eccentric binaries of black holes and neutron stars can form through various n-body interactions. Such a binary could emit a significant fraction of its binding energy in a sequence of largely isolated gravitational-wave bursts prior to merger. Given expected black hole and neutron star masses, many such systems will emit these repeated bursts at frequencies within the sensitive band of contemporary ground-based gravitational-wave detectors. Unfortunately, existing gravitational-wave searches are ill suited to detect these signals. In this work, we adapt a "power stacking" method to the detection of gravitational-wave signals from highly eccentric binaries. We implement this method as an extension of the Q transform, a projection onto a multiresolution basis of windowed complex exponentials that has previously been used to analyze data from the network of LIGO/Virgo detectors. Our method searches for excess power over an ensemble of time-frequency tiles. We characterize the performance of our method using Monte Carlo experiments with signals injected in simulated detector noise. Our results indicate that the power stacking method achieves substantially better sensitivity to eccentric binary signals than existing localized burst searches.
AB - In dense stellar regions, highly eccentric binaries of black holes and neutron stars can form through various n-body interactions. Such a binary could emit a significant fraction of its binding energy in a sequence of largely isolated gravitational-wave bursts prior to merger. Given expected black hole and neutron star masses, many such systems will emit these repeated bursts at frequencies within the sensitive band of contemporary ground-based gravitational-wave detectors. Unfortunately, existing gravitational-wave searches are ill suited to detect these signals. In this work, we adapt a "power stacking" method to the detection of gravitational-wave signals from highly eccentric binaries. We implement this method as an extension of the Q transform, a projection onto a multiresolution basis of windowed complex exponentials that has previously been used to analyze data from the network of LIGO/Virgo detectors. Our method searches for excess power over an ensemble of time-frequency tiles. We characterize the performance of our method using Monte Carlo experiments with signals injected in simulated detector noise. Our results indicate that the power stacking method achieves substantially better sensitivity to eccentric binary signals than existing localized burst searches.
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U2 - 10.1103/PhysRevD.90.103001
DO - 10.1103/PhysRevD.90.103001
M3 - Article
AN - SCOPUS:84911945479
SN - 1550-7998
VL - 90
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 10
M1 - 103001
ER -