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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 …
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…
Large-mass neutron stars with hyperonization
Wei-Zhou Jiang, Bao-An Li, Lie-Wen Chen
Within a density-dependent relativistic mean-field model using in-medium meson-hadron coupling constants and meson masses, we explore effects of in-medium hyperon interactions on p…
Nuclear constraints on non-Newtonian gravity at femtometer scale
Jun Xu, Bao-An Li, Lie-Wen Chen +1
Effects of the non-Newtonian gravity on properties of finite nuclei are studied by consistently incorporating both the direct and exchange contribution of the Yukawa potential in t…
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…
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…