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• W2006035641 abstract "We analyze the distinguishability of populations of coalescing binary neutron stars, neutron-star black-hole binaries, and binary black holes, whose gravitational-wave signatures are expected to be observed by the advanced network of ground-based interferometers LIGO and Virgo. We consider population-synthesis predictions for plausible merging binary distributions in mass space, along with measurement accuracy estimates from the main gravitational-wave parameter-estimation pipeline. We find that for our model compact-object binary mass distribution, we can always distinguish binary neutron stars and black-hole--neutron-star binaries, but not necessarily black-hole--neutron-star binaries and binary black holes; however, with a few tens of detections, we can accurately identify the three subpopulations and measure their respective rates." @default.
• W2006035641 created "2016-06-24" @default.
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• W2006035641 date "2015-05-01" @default.
• W2006035641 modified "2023-09-25" @default.
• W2006035641 title "Distinguishing types of compact-object binaries using the gravitational-wave signatures of their mergers" @default.
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• W2006035641 doi "https://doi.org/10.1093/mnrasl/slv054" @default.
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