William G. Newton

Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae

William G. Newton, J. R. Stone · Physical Review C · 2009 · 170 citations

Uniform Nuclear Matter, Engineering, Nuclear Physics +15

Using neutron star observations to determine crust thicknesses, moments of inertia, and tidal deformabilities

Andrew W. Steiner, Stefano Gandolfi, F. J. Fattoyev et al. · Physical Review C · 2015 · 161 citations · Full text

Relativistic Astrophysics, Neutron Star Physics, Crustal Deformation +15

Dense nuclear matter equation of state from heavy-ion collisions

Agnieszka Sorensen, Kshitij Agarwal, K. W. Brown et al. · Progress in Particle and Nuclear Physics · 2023 · 153 citations · Full text

Heavy Ion Physic, High-energy Nuclear Reaction, Nuclear Physics +6

Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars

F. J. Fattoyev, J. Carvajal, William G. Newton et al. · Physical Review C · 2013 · 148 citations · Full text

A SURVEY OF THE PARAMETER SPACE OF THE COMPRESSIBLE LIQUID DROP MODEL AS APPLIED TO THE NEUTRON STAR INNER CRUST

William G. Newton, Michael Gearheart, Bao-An Li · The Astrophysical Journal Supplement Series · 2012 · 111 citations · Full text