189 citations · 1.4k across the 33 of their papers we have counts for
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Constraining Nuclear Symmetry Energy with Multi-messenger Resonant Shattering Flares
Duncan Neill, Rebecca Preston, William G. Newton +1
Much effort is devoted to measuring the nuclear symmetry energy through neutron star (NS) and nuclear observables. Since matter in the NS core may be non-hadronic, observables like…
Resonant Shattering Flares in Black Hole-Neutron Star and Binary Neutron Star Mergers
Duncan Neill, David Tsang, Hendrik van Eerten +2
Resonant Shattering flares (RSFs) are bursts of gamma-rays expected to be triggered by tidal resonance of a neutron star (NS) during binary inspiral. They are strongly dependent on…
Resonant Shattering Flares as Multimessenger Probes of the Nuclear Symmetry Energy
Duncan Neill, William G. Newton, David Tsang
The behaviour of the nuclear symmetry energy near saturation density is important for our understanding of dense nuclear matter. This density dependence can be parameterised by the…
Prior probability distributions of neutron star crust models
Lauren Balliet, William Newton, Sarah Cantu +1
To make best use of multi-faceted astronomical and nuclear data-sets, probability distributions of neutron star models that can be used to propagate errors consistently from one do…
The state of matter in simulations of core-collapse supernovae -- Reflections and recent developments
Tobias Fischer, Niels-Uwe Bastian, David Blaschke +7
In this review article we discuss selected developments regarding the role of the equation of state (EOS) in simulations of core-collapse supernovae. There are no first-principle c…
Nuclear pasta and supernova neutrinos at late times
C. J. Horowitz, D. K. Berry, M. E. Caplan +5
Nuclear pasta, with nucleons arranged into tubes, sheets, or other complex shapes, is expected in core collapse supernovae (SNe) at just below nuclear density. We calculate the add…