Investigation into the properties and structure of unstable nuclei far from stability is a key
avenue of research in modern nuclear physics. These efforts are motivated by the continual …

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

In recent years our understanding of the dense matter equation of state (EOS) of neutron
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …

We introduce a new framework for quantifying correlated uncertainties of the infinite-matter
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …

Is the secondary component of GW190814 the lightest black hole or the heaviest neutron
star ever discovered in a double compact-object system [Abbott et al. Astrophys. J. 896, L44 …

Collinear laser spectroscopy is performed on the nickel isotopes Ni 58-68, 70, using a time-
resolved photon counting system. From the measured isotope shifts, nuclear charge radii R …

Nuclear charge radii of Ni 55, 56 were measured by collinear laser spectroscopy. The
obtained information completes the behavior of the charge radii at the shell closure of the …

We compute the charge radii and ground-state energies of even-mass neon and
magnesium isotopes from neutron number N= 8 to the dripline. Our calculations are based …

Isotope shifts of Ra 223–226, 228 F 19 were measured for different vibrational levels in the
electronic transition A 2 Π 1/2← X 2 Σ+. The observed isotope shifts demonstrate the …

The neutron skin of atomic nuclei impacts the structure of neutron-rich nuclei, the equation of
state of nucleonic matter, and the size of neutron stars. Here we predict the neutron skin of …