55 citations · 196 across the 11 of their papers we have counts for
11 papers
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…
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…
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)…
A luminous precursor in the extremely bright GRB 230307A
S. Dichiara, D. Tsang, E. Troja +3
GRB 230307A is an extremely bright long duration GRB with an observed gamma-ray fluence of 310 erg cm (10-1000 keV), second only to GRB 221009A. Desp…
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…
The Hydrogen-Poor Superluminous Supernovae from the Zwicky Transient Facility Phase-I Survey: II. Light Curve Modeling and Characterization of Undulations
Z. H. Chen, Lin Yan, T. Kangas +19
We present analysis of the light curves (LCs) of 77 hydrogen-poor superluminous supernovae (SLSNe-I) discovered during the Zwicky Transient Facility Phase-I operation. We find that…
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…
SN 2017gci: a nearby Type I Superluminous Supernova with a bumpy tail
Achille Fiore, Ting-Wan Chen, Anders Jerkstrand +26
We present and discuss the optical spectro-photometric observations of the nearby (z=0.087) Type I superluminous supernova (SLSN I) SN 2017gci, whose peak K-corrected absolute magn…
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…
Impact of statistical uncertainties on the composition of the outer crust of a neutron star
A. Pastore, D. Neill, H. Powell +2
By means of Monte Carlo methods, we perform a full error analysis on the Duflo-Zucker mass model. In particular, we study the presence of correlations in the residuals to obtain a…
Impact of error analysis on the composition the outer crust of a neutron star
D Neill, K Medler, A Pastore +1
By means of bootstrap technique, we perform a full error analysis on the Duflo-Zucker mass model. We illustrate the impact of such study on the predicted chemical composition of th…