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

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nucl-th2023★ 189 cited

Dense Nuclear Matter Equation of State from Heavy-Ion Collisions

Agnieszka Sorensen, Kshitij Agarwal, Kyle W. Brown +133

The nuclear equation of state (EOS) is at the center of numerous theoretical and experimental efforts in nuclear physics. With advances in microscopic theories for nuclear interact…

nucl-th2021★ 16 cited

From neutron skins and neutron matter to the neutron star crust

William G. Newton, Rebecca Preston, Lauren Balliet +1

We present the first Bayesian inference of neutron star crust properties to incorporate neutron skin data, including the recent PREX measurement of the neutron skin of Pb,…

nucl-th2021★ 26 cited

Glassy quantum nuclear pasta in neutron star crusts

William G. Newton, Mark Alexander Kaltenborn, Sarah Cantu +3

We investigate the nuclear pasta phases in neutron star crusts by conducting a large number of three-dimensional Hartree-Fock+BCS calculations at densities leading to the crust-cor…

nucl-th2020★ 36 cited

The nuclear symmetry energy from neutron skins and pure neutron matter in a Bayesian framework

William G. Newton, Gabriel Crocombe

We present an inference of the nuclear symmetry energy magnitude , the slope and the curvature by combining neutron skin data on Ca, Pb and Sn isotopes and our…

nucl-th2017★ 61 cited

How tightly is nuclear symmetry energy constrained by unitary Fermi gas?

Nai-Bo Zhang, Bao-Jun Cai, Bao-An Li +2

We examine critically how tightly the density dependence of nuclear symmetry energy \esym is constrained by the universal equation of state (EOS) of the unitary Fermi gas $E_{\rm{U…

nucl-th2015★ 51 cited

Constraints on the symmetry energy from observational probes of the neutron star crust

William G. Newton, Joshua Hooker, Michael Gearheart +4

A number of observed phenomena associated with individual neutron star systems or neutron star populations find explanations in models in which the neutron star crust plays an impo…