Inferring neutron star properties from GW170817 with universal relations

Because all neutron stars share a common equation of state, tidal deformability constraints from the compact binary coalescence GW170817 have implications for the properties of neutron stars in other systems. Using equation-of-state insensitive relations between macroscopic observables like moment of inertia (I), tidal deformability (Lambda) and stellar compactness, we derive constraints on these properties as a function of neutron star mass based on the LIGO-Virgo Collaboration's canonical deformability measurement, Lambda(1.4) = 190(-120)(+390). Specific estimates of Lambda, I, dimensionless spin chi, and stellar radius R for a few systems targeted by radio or x-ray studies are extracted from the general constraints. We also infer the canonical neutron star radius as R-1.4 = 10.9(-1.5)(+1.9) km at 90% confidence. We further demonstrate how a gravitational-wave measurement of Lambda(1.4) can be combined with independent measurements of neutron star radii to tighten constraints on the tidal deformability as a proxy for the equation of state. We find that GW170817 and existing observations of six thermonuclear bursters in low-mass x-ray binaries jointly imply Lambda(1.4) = 196(-63)(+92) at the 90% confidence level.