3 papers
astro-ph.HE2026
Measuring radii of merging neutron stars with interface-mode asteroseismology informed by nuclear theory and experiment
Duncan Neill, William G. Newton, Jeremy W. Holt +3
The structure and dynamics of neutron stars can be used to probe the physics of extreme matter at nuclear densities and beyond. Nucleonic matter up to ~2-3 times nuclear saturation…
astro-ph.HE2024
Resonant shattering flares as asteroseismic tests of chiral effective field theory
Duncan Neill, David Tsang, Christian Drischler +2
Chiral effective field theory (EFT) has proved to be a powerful microscopic framework for predicting the properties of neutron-rich nuclear matter with quantified theoretical un…
astro-ph.HE2024
Strengthening nuclear symmetry energy constraints using multiple resonant shattering flares of neutron stars with realistic mass uncertainties
Duncan Neill, David Tsang, William G. Newton
With current and planned gravitational-wave (GW) observing runs, coincident multimessenger timing of Resonant Shattering Flares (RSFs) and GWs may soon allow for neutron star (NS)…