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 …

The atomic nucleus is a quantum many-body system whose constituent nucleons (protons
and neutrons) are subject to complex nucleon-nucleon interactions that include spin-and …

We report a quantum simulation of the deuteron binding energy on quantum processors
accessed via cloud servers. We use a Hamiltonian from pionless effective field theory at …

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 …

Ground-state properties of even–even nuclei with 8≤ Z≤ 120 from the proton drip line to the
neutron drip line have been investigated using the deformed relativistic Hartree–Bogoliubov …

Despite being a complex many-body system, the atomic nucleus exhibits simple structures
for certain 'magic'numbers of protons and neutrons. The calcium chain in particular is both …

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 …

By taking into account the surface diffuseness correction for unstable nuclei, the accuracy of
the macroscopic–microscopic mass formula is further improved. The rms deviation with …

In the past decade, coupled-cluster theory has seen a renaissance in nuclear physics, with
computations of neutron-rich and medium-mass nuclei. The method is efficient for nuclei …

What is the size of the atomic nucleus? This deceivably simple question is difficult to answer.
Although the electric charge distributions in atomic nuclei were measured accurately already …