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BinarySkyHough: a new method to search for continuous gravitational waves from unknown neutron stars in binary systems

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arxiv 1904.04873 v2 pith:SCLEQQBG submitted 2019-04-09 astro-ph.IM gr-qc

classification astro-ph.IMgr-qc
keywords pipelinebinaryneutronstarssystemsbinaryskyhoughcontinuousgravitational
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Non-axysymmetric, fast-spinning unknown neutron stars in binary systems may emit continuous gravitational waves (nearly-monochromatic long-duration signals) which can be detected by ground-based detectors like LIGO and Virgo. In this paper we present a new pipeline, called $\textit{BinarySkyHough}$, that can carry out all-sky searches for neutron stars in binary systems by exploiting the usage of graphics processing units. We give a detailed explanation of this new pipeline, and we present simulations which allow us to estimate the sensitivity of the new pipeline, which is approximately twice as sensitive as the best active pipeline with a comparable computational cost.

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  1. One-stop strategy to search for long-duration gravitational-wave signals

    gr-qc 2024-11 conditional novelty 6.0 of 10

    A generic GPU search engine plus a fast semianalytic sensitivity estimator could make blind continuous gravitational-wave searches much cheaper to run and characterize.

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