Asteroseismic crust-core interface mode frequency infers neutron star radius to 5-10% if low-density physics is known, measurable via resonant shattering flares or next-gen GW detectors.
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Measuring the radii of merging neutron stars with asteroseismology
Asteroseismic crust-core interface mode frequency infers neutron star radius to 5-10% if low-density physics is known, measurable via resonant shattering flares or next-gen GW detectors.