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- W3100494057 abstract "We present the prospects for the early (pre-merger) detection and localization of compact-binary coalescences using gravitational waves over the next 10 years. Early warning can enable the direct observation of the prompt and early electromagnetic emission of a neutron star merger. We examine the capabilities of the ground based detectors at their Design sensitivity (2021-2022), the planned A+ upgrade (2024-2026), and the envisioned Voyager concept (late 2020's). We find that for a fiducial rate of binary neutron star mergers of $1000 ~mathrm{Gpc}^{-3} mathrm{yr}^{-1}$, the Design, A+, and Voyager era networks can provide 18, 54, and 195s of warning for one source per year of observing, respectively, with a sky localization area $<$100 deg$^2$ at a $90%$ credible level. At the same rate, the A+ and Voyager era networks will be able to provide 9 and 43s of warning, respectively, for a source with $<$10 deg$^2$ localization area. We compare the idealized search sensitivity to that achieved by the PyCBC Live search tuned for pre-merger detection. The gravitational-wave community will be prepared to produce pre-merger alerts. Our results motivate the operation of observatories with wide fields-of-view, automation, and the capability for fast slewing to observe simultaneously with the gravitational-wave network." @default.
- W3100494057 created "2020-11-23" @default.
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- W3100494057 date "2020-10-16" @default.
- W3100494057 modified "2023-10-16" @default.
- W3100494057 title "Gravitational-wave Merger Forecasting: Scenarios for the Early Detection and Localization of Compact-binary Mergers with Ground-based Observatories" @default.
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- W3100494057 doi "https://doi.org/10.3847/2041-8213/abbc10" @default.
- W3100494057 hasPublicationYear "2020" @default.
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