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

ligo Scientific Collaboration, Virgo Collaboration

Research output: Contribution to journalArticlepeer-review

Abstract

One unanswered question about the binary neutron star coalescence GW170817 is the nature of its postmerger 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 (US)
JournalUnknown Journal
StatePublished - Oct 5 2018

Keywords

  • Data analysis – stars
  • Gravitational waves – methods
  • Neutron

ASJC Scopus subject areas

  • General

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