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Astrophysical science metrics for next-generation gravitational-wave detectors

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arxiv 1905.02842 v3 pith:VGPG2OWL submitted 2019-05-07 astro-ph.HE gr-qcphysics.ins-det

Rana X Adhikari , P Ajith , Yanbei Chen , James A Clark , Vladimir Dergachev , Nicolas V Fotopoulos , Sarah E. Gossan , Ilya Mandel
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Maria Okounkova Vivien Raymond Jocelyn S Read
This is my paper · ORCID
classification astro-ph.HEgr-qcphysics.ins-det
keywords gravitational-wavemetricsdetectordetectorsanalysesastronomyastrophysicalastrophysically
verification ladder T0 review T1 audit T2 compute T3 formal

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The second generation of gravitational-wave detectors are being built and tuned all over the world. The detection of signals from binary black holes is beginning to fulfill the promise of gravitational-wave astronomy. In this work, we examine several possible configurations for third-generation laser interferometers in existing km-scale facilities. We propose a set of astrophysically motivated metrics to evaluate detector performance. We measure the impact of detector design choices against these metrics, providing a quantitative cost-benefit analyses of the resulting scientific payoffs.

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  1. Searching for ultralight bosons within spin measurements of a population of binary black hole mergers

    gr-qc 2019-08 conditional novelty 6.0 of 10

    A hierarchical Bayesian analysis of mock binary black hole populations shows that roughly a hundred high-signal-to-noise mergers could exclude or confirm ultralight bosons in the 1e-13 to 3e-12 eV range.

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