activity
19932024
most citedEquation of state and neutron star properties constrained by nuclear physics and observation

764 citations · 5.8k across the 87 of their papers we have counts for

collaborators

87 papers

nucl-th2024

Multicomponent Fermi systems at low densities

C. J. Pethick, A. Schwenk

We calculate, to second order in the scattering length between two fermions, the Landau quasiparticle interaction for a low-density mixture of two fermion species with unequal dens…

hep-ph2024

Understanding the puzzle of angular momentum conservation in beta decay and related processes

Gordon Baym, Jen-Chieh Peng, C. J. Pethick

We ask the question of how angular momentum is conserved in electroweak interaction processes. To introduce the problem with a minimum of mathematics, we first raise the same issue…

nucl-th2021★ 2 cited

Superfluid density in disordered pasta phases in neutron star crusts

Zhao-Wen Zhang, C. J. Pethick

We calculate the superfluid density of nucleons in disordered pasta phases in the inner crust of neutron stars using an effective medium approach which parallels that previously us…

nucl-th2020★ 8 cited

Proton superconductivity in pasta phases in neutron star crusts

Zhao-Wen Zhang, C. J. Pethick

In the so-called pasta phases predicted to occur in neutron star crusts, protons are able to move easily over large distances because the nuclear matter regions are extended in spa…

astro-ph.HE2020★ 77 cited

Equation of state constraints from nuclear physics, neutron star masses, and future moment of inertia measurements

S. K. Greif, K. Hebeler, J. M. Lattimer +2

We explore constraints on the equation of state (EOS) of neutron-rich matter based on microscopic calculations up to nuclear densities and observations of neutron stars. In a previ…

cond-mat.mtrl-sci2020★ 35 cited

Elastic properties of phases with nonspherical nuclei in dense matter

C. J. Pethick, Zhaowen Zhang, D. N. Kobyakov

We consider the elastic constants of phases with nonspherical nuclei, so-called pasta phases, predicted to occur in the inner crust of a neutron star. First, we treat perfectly ord…