Searching for Gravitational Waves from Compact Binaries with Precessing Spins
Ian Harry, Stephen Privitera, Alejandro Boh\'e, Alessandra Buonanno

TL;DR
This paper develops a new search method for gravitational waves from precessing binary systems, improving detection sensitivity for systems with high spin misalignment, especially for neutron-star--black-hole mergers.
Contribution
It introduces a new statistic and template banks for generic precessing spins, enhancing gravitational wave detection capabilities beyond aligned-spin models.
Findings
Improved signal recovery for high-mass ratio, precessing systems up to 60%.
Generic-spin banks increase templates by a factor of 10-20.
Small sensitivity loss (~4%) for well-covered aligned-spin systems.
Abstract
Current searches for gravitational waves from compact-object binaries with the LIGO and Virgo observatories employ waveform models with spins aligned (or anti-aligned) with the orbital angular momentum. Here, we derive a new statistic to search for compact objects carrying generic (precessing) spins. Applying this statistic, we construct banks of both aligned- and generic-spin templates for binary black holes and neutron-star--black-hole binaries, and compare the effectualness of these banks towards simulated populations of generic-spin systems. We then use these banks in a pipeline analysis of Gaussian noise to measure the increase in background incurred by using generic- instead of aligned-spin banks. Although the generic-spin banks have a factor of ten to twenty more templates than the aligned-spin banks, we find an overall improvement in signal recovery at fixed false-alarm rate for…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Cosmology and Gravitation Theories
