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- W2058184357 abstract "We study the possibility of pre-merger localization of eccentric compact binary coalescences by second-generation gravitational-wave detector networks. Gravitational waves from eccentric binaries can be regarded as a sequence of pulses, which are composed of various higher harmonic modes than ones with twice the orbital frequency. The higher harmonic modes from a very early inspiral phase will not only contribute to the signal-to-noise ratio, but also allow us to localize the gravitational-wave source before the merger sets in. This is due to the fact that high-frequency gravitational waves are essential for the source localization via triangulation by ground-based detector networks. We found that the single-detector signal-to-noise ratio exceeds 5 at 10 min before the merger for a 1.4–1.4 M⊙ eccentric binary neutron stars at 100 Mpc in optimal cases, and it can be localized up to 10 deg2 at half a minute before the merger by a four-detector network. We will even be able to achieve ∼10 deg2 at 10 min before the merger for a face-on eccentric compact binary by a five-detector network." @default.
- W2058184357 created "2016-06-24" @default.
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- W2058184357 date "2014-05-15" @default.
- W2058184357 modified "2023-10-18" @default.
- W2058184357 title "Pre-merger localization of eccentric compact binary coalescences with second-generation gravitational-wave detector networks" @default.
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- W2058184357 doi "https://doi.org/10.1093/mnras/stu698" @default.
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