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Journal Article

Impact of precession on aligned-spin searches for neutron-tar-black-hole binaries

MPS-Authors
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Lundgren,  Andrew
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Nielsen,  A. B.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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1411.6815.pdf
(Preprint), 4MB

PhysRevD.91.pdf
(Any fulltext), 4MB

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Citation

Dal Canton, T., Lundgren, A., & Nielsen, A. B. (2015). Impact of precession on aligned-spin searches for neutron-tar-black-hole binaries. Physical Review D, 91: 062010. doi:10.1103/PhysRevD.91.062010.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0024-C656-0
Abstract
The inclusion of aligned-spin effects in gravitational-wave search pipelines for neutron-star--black-hole binary coalescence has been shown to increase the astrophysical reach with respect to search methods where spins are neglected completely, under astrophysically reasonable assumptions about black-hole spins. However, theoretical considerations and population synthesis models suggest that many of these binaries may have a significant misalignment between the black-hole spin and the orbital angular momentum, which could lead to precession of the orbital plane during the inspiral and a consequent loss in detection efficiency if precession is ignored. This work explores the effect of spin misalignment on a search pipeline that completely neglects spin effects and on a recently-developed pipeline that only includes aligned-spin effects. Using synthetic but realistic data, which could reasonably represent the first scientific runs of advanced-LIGO detectors, the relative sensitivities of both pipelines are shown for different assumptions about black-hole spin magnitude and alignment with the orbital angular momentum. Despite the inclusion of aligned-spin effects, the loss in signal-to-noise ratio due to precession can be as large as $40\%$, but this has a limited impact on the overall detection rate: even if precession is a predominant feature of neutron-star--black-hole binaries, an aligned-spin search pipeline can still detect at least half of the signals compared to an idealized generic precessing search pipeline.