Neutron Star Merger Remnants: Braking Indices, Gravitational Waves, and the Equation Of State
Published in AIP Conference Proceedings, 2019
Recommended citation: Lasky et al. (2019) https://ui.adsabs.harvard.edu/abs/2019arXiv190501387L/abstract
Abstract: The binary neutron star merger GW170817/GRB170817A confirmed that at least some neutron star mergers are the progenitors of short gamma-ray bursts. Many short gamma-ray bursts have long-term x-ray afterglows that have been interpreted in terms of post-merger millisecond magnetars—rapidly rotating, highly magnetised, massive neutron stars. We review our current understanding of millisecond magnetars born in short gamma-ray bursts, focusing particularly three main topics. First, whether millisecond magnetars really do provide the most plausible explain for the x-ray plateau. Second, determining and observing the gravitational-wave emission from these remnants. Third, determining the equation of state of nuclear matter from current and future x-ray and gravitational-wave measurements.