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Search for gravitational waves from a long-lived remnant of the binary neutron star merger GW170817

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One unanswered question about the binary neutron star coalescence GW170817 is the nature of its post-merger remnant. A previous search for post-merger gravitational waves targeted high-frequency signals from a possible neutron star remnant with a maximum signal duration of 500 s. Here we revisit the neutron star remnant scenario with a focus on longer signal durations up until the end of the Second Advanced LIGO-Virgo Observing run, 8.5 days after the coalescence of GW170817. The main physical scenario for such emission is the power-law spindown of a massive magnetar-like remnant. We use four independent search algorithms with varying degrees of restrictiveness on the signal waveform and different ways of dealing with noise artefacts. In agreement with theoretical estimates, we find no significant signal candidates. Through simulated signals, we quantify that with the current detector sensitivity, nowhere in the studied parameter space are we sensitive to a signal from more than 1 Mpc away, compared to the actual distance of 40 Mpc. This study however serves as a prototype for post-merger analyses in future observing runs with expected higher sensitivity.
Original languageEnglish
Article number160
Number of pages19
JournalThe Astrophysical Journal
Volume875
Issue number2
DOIs
Publication statusPublished - 25 Apr 2019

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  • Abbott_2019_ApJ_875_160

    Rights statement: B. P. Abbott et al. 2019 ApJ 875:160. © 2019 The American Astronomical Society. All rights reserved. Reproduced by permission of the AAS.

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