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 …

A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

The nuclear matrix elements that govern the rate of neutrinoless double beta decay must be
accurately calculated if experiments are to reach their full potential. Theorists have been …

Over the last decade, new developments in Similarity Renormalization Group techniques
and nuclear many-body methods have dramatically increased the capabilities of ab initio …

Quantum Monte Carlo methods have proved valuable to study the structure and reactions of
light nuclei and nucleonic matter starting from realistic nuclear interactions and currents …

Microscopic calculations of neutron matter based on nuclear interactions derived from chiral
effective field theory, combined with the recent observation of a 1.97±0.04 M☉ neutron star …

We optimize Δ-full nuclear interactions from chiral effective field theory. The low-energy
constants of the contact potentials are constrained by two-body scattering phase shifts, and …

The symmetry energy contribution to the nuclear equation of state impacts various
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …

With the goal of develo** predictive ab initio capability for light and medium-mass nuclei,
two-nucleon and three-nucleon forces from chiral effective field theory are optimized …