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• W2301375440 abstract "Recent non-detection of gravitational-wave backgrounds from pulsar timing arrays casts further uncertainty on the evolution of supermassive black hole binaries. We study the capabilities of current gravitational-wave observatories to detect individual binaries and demonstrate that, contrary to conventional wisdom, some are in principle detectable throughout the Universe. In particular, a binary with rest-frame mass $gtrsim10^{10},M_odot$ can be detected by current timing arrays at arbitrarily high redshifts. The same claim will apply for less massive binaries with more sensitive future arrays. As a consequence, future searches for nanohertz gravitational waves could be expanded to target evolving high-redshift binaries. We calculate the maximum distance at which binaries can be observed with pulsar timing arrays and other detectors, properly accounting for redshift and using realistic binary waveforms." @default.
• W2301375440 created "2016-06-24" @default.
• W2301375440 creator A5000611658 @default.
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• W2301375440 date "2016-03-10" @default.
• W2301375440 modified "2023-10-16" @default.
• W2301375440 title "Detectability of Gravitational Waves from High-Redshift Binaries" @default.
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• W2301375440 doi "https://doi.org/10.1103/physrevlett.116.101102" @default.
• W2301375440 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/27015470" @default.
• W2301375440 hasPublicationYear "2016" @default.
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