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arXiv · 1905.01387

Neutron Star Merger Remnants: Braking Indices, Gravitational Waves, and the Equation Of State

Paul D. Lasky·Nikhil Sarin·Greg Ashton
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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.

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Paul D. Lasky, Nikhil Sarin, Greg Ashton. 2019-05-03. Neutron Star Merger Remnants: Braking Indices, Gravitational Waves, and the Equation Of State. https://doi.org/10.1063/1.5117815

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