Constraining the gravitational-wave afterglow from a binary neutron star coalescence

Sharan Banagiri, Michael W. Coughlin, James Clark, Paul D. Lasky, M. A. Bizouard, Colm Talbot, Eric Thrane, Vuk Mandic

Research output: Contribution to journalArticlepeer-review

14 Scopus citations

Abstract

Binary neutron star mergers are rich laboratories for physics, accessible with ground-based interferometric gravitational-wave detectors such as the Advanced LIGO and Advanced Virgo. If a neutron star remnant survives the merger, it can emit gravitational waves that might be detectable with the current or next generation detectors. The physics of the long-lived post-merger phase is not well understood and makes modelling difficult. In particular the phase of the gravitational-wave signal is not well modelled. In this paper, we explore methods for using long duration post-merger gravitational-wave signals to constrain the parameters and the properties of the remnant. We develop a phase-agnostic likelihood model that uses only the spectral content for parameter estimation and demonstrate the calculation of a Bayesian upper limit in the absence of a signal. With the millisecond magnetar model, we show that for an event like GW170817, the ellipticity of a long-lived remnant can be constrained to less than about 0.5 in the parameter space used.

Original languageEnglish (US)
Pages (from-to)4945-4951
Number of pages7
JournalMonthly Notices of the Royal Astronomical Society
Volume492
Issue number4
DOIs
StatePublished - 2020

Bibliographical note

Publisher Copyright:
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Keywords

  • Gravitational waves
  • Methods: statistical
  • Stars: neutron

Fingerprint

Dive into the research topics of 'Constraining the gravitational-wave afterglow from a binary neutron star coalescence'. Together they form a unique fingerprint.

Cite this