activity
20032023
most citedDense Nuclear Matter Equation of State from Heavy-Ion Collisions

189 citations · 1.4k across the 33 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2016★ 8 cited

Testing the formation scenarios of binary neutron star systems with measurements of the neutron star moment of inertia

William G. Newton, Andrew W. Steiner, Kent Yagi

Two low mass neutron stars, J0737-3039B and the companion to J1756-2251, show strong evidence of being formed from the collapse of an ONeMg core in an electron capture supernova (E…

astro-ph.SR2015★ 35 cited

Observational constraints on neutron star crust-core coupling during glitches

William G. Newton, Sabrina Berger, Brynmor Haskell

We demonstrate that observations of glitches in the Vela pulsar can be used to investigate the strength of the crust-core coupling in a neutron star, and suggest that recovery from…

astro-ph.SR2013★ 40 cited

The cooling of the Cassiopeia A neutron star as a probe of the nuclear symmetry energy and nuclear pasta

William G. Newton, Kyleah Murphy, Joshua Hooker +1

X-ray observations of the neutron star in the Cas A supernova remnant over the past decade suggest the star is undergoing a rapid drop in surface temperature of …

astro-ph.SR2013★ 26 cited

Efficacy of crustal superfluid neutrons in pulsar glitch models

J. Hooker, W. G. Newton, Bao-An Li

In order to assess the ability of purely crust-driven glitch models to match the observed glitch activity in the Vela pulsar, we conduct a systematic analysis of the dependence of…

astro-ph.SR2011★ 6 cited

The nuclear symmetry energy, the inner crust, and global neutron star modeling

William G. Newton, Michael Gearheart, Josh Hooker +1

The structure and composition of the inner crust of neutron stars, as well as global stellar properties such as radius and moment of inertia, have been shown to correlate with para…

astro-ph.SR2011★ 49 cited

Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy

De-Hua Wen, W. G. Newton, Bao-An Li

Using a simple model of a neutron star with a perfectly rigid crust constructed and a set of crust and core equations of state that span the range of nuclear experimental uncertain…