Charles Horowitz

TL;DR: An accurate measurement of the neutron radius in 208Pb-via parity violating electron scattering-may have important implications for the structure of the crust of neutron stars.

TL;DR: In this paper, the authors examined the results of laboratory experiments that have provided initial constraints on the nuclear symmetry energy and on its density dependence at and somewhat below normal nuclear matter density.

TL;DR: In this article, Liu and Siegbahn made an accurate least square fit to the potential energy surface start for H+H2 with a root-mean-square error of 0.17 kcal/mol.

TL;DR: The relativistic Hartree equations for spherical nuclei were derived from a relativistically nuclear quantum field theory using a coordinate-space Green function approach in this paper, which represented the mean-field approximation for a finite nuclear system.

TL;DR: Ab et al. as mentioned in this paper used a set of realistic models of the equation of state (EOS) that yield an accurate description of the properties of finite nuclei, support neutron stars of two solar masses, and provide a Lorentz covariant extrapolation to dense matter are used to confront its predictions against gravitational-wave data.