| The double pulsar J0737-3039: testing the neutron star equation of state P Podsiadlowski, JDM Dewi, P Lesaffre, JC Miller, WG Newton, JR Stone Monthly Notices of the Royal Astronomical Society 361 (4), 1243-1249, 2005 | 173 | 2005 |
| Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae WG Newton, JR Stone Physical Review C 79 (5), 055801, 2009 | 164 | 2009 |
| Using neutron star observations to determine crust thicknesses, moments of inertia, and tidal deformabilities AW Steiner, S Gandolfi, FJ Fattoyev, WG Newton Physical Review C 91 (1), 015804, 2015 | 126 | 2015 |
| Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars FJ Fattoyev, J Carvajal, WG Newton, BA Li Physical Review C 87 (1), 015806, 2013 | 124 | 2013 |
| Upper limits on the observational effects of nuclear pasta in neutron stars M Gearheart, WG Newton, J Hooker, BA Li Monthly Notices of the Royal Astronomical Society, 2011 | 106 | 2011 |
| Critical density and impact of Δ (1232) resonance formation in neutron stars BJ Cai, FJ Fattoyev, BA Li, WG Newton Physical Review C 92 (1), 015802, 2015 | 105 | 2015 |
| A survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crust WG Newton, M Gearheart, BA Li The Astrophysical Journal Supplement Series 204 (1), 9, 2012 | 104 | 2012 |
| Neutron–proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon–nucleus scattering data within an isospin dependent optical model XH Li, WJ Guo, BA Li, LW Chen, FJ Fattoyev, WG Newton Physics Letters B 743, 408-414, 2015 | 80 | 2015 |
| Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of state FJ Fattoyev, WG Newton, J Xu, BA Li Physical Review C 86 (2), 025804, 2012 | 66 | 2012 |
| How sensitive is the neutron star r-mode instability window to the density dependence of nuclear symmetry energy? DH Wen, WG Newton, BA Li Arxiv preprint arXiv:1110.5985, 2011 | 65 | 2011 |
| How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas? NB Zhang, BJ Cai, BA Li, WG Newton, J Xu Nuclear Science and Techniques 28 (12), 181, 2017 | 61 | 2017 |
| Constraints on the symmetry energy from observational probes of the neutron star crust WG Newton, J Hooker, M Gearheart, K Murphy, DH Wen, FJ Fattoyev, ... The European Physical Journal A 50, 1-19, 2014 | 58 | 2014 |
| Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data WG Newton, BA Li Physical Review C 80 (6), 065809, 2009 | 51 | 2009 |
| Impact of the equation-of-state–gravity degeneracy on constraining the nuclear symmetry energy from astrophysical observables XT He, FJ Fattoyev, BA Li, WG Newton Physical Review C 91 (1), 015810, 2015 | 45 | 2015 |
| The cooling of the Cassiopeia A neutron star as a probe of the nuclear symmetry energy and nuclear pasta WG Newton, K Murphy, J Hooker, BA Li The Astrophysical Journal Letters 779 (1), L4, 2013 | 42 | 2013 |
| The state of matter in simulations of core-collapse supernovae—Reflections and recent developments T Fischer, NU Bastian, D Blaschke, M Cierniak, M Hempel, T Klähn, ... Publications of the Astronomical Society of Australia 34, e067, 2017 | 39 | 2017 |
| Observational constraints on neutron star crust–core coupling during glitches WG Newton, S Berger, B Haskell Monthly Notices of the Royal Astronomical Society 454 (4), 4400-4410, 2015 | 39 | 2015 |
| Probing the high-density behavior of symmetry energy with gravitational waves FJ Fattoyev, WG Newton, BA Li The European Physical Journal A 50, 1-13, 2014 | 36 | 2014 |
| Dense nuclear matter equation of state from heavy-ion collisions A Sorensen, K Agarwal, KW Brown, Z Chajęcki, P Danielewicz, ... Progress in Particle and Nuclear Physics 134, 104080, 2024 | 34 | 2024 |
| Nuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian framework WG Newton, G Crocombe Physical Review C 103 (6), 064323, 2021 | 32 | 2021 |
