The last decade has witnessed both quantitative and qualitative progress in shell-model
studies, which have resulted in remarkable gains in our understanding of the structure of the …

The r-process, or the rapid neutron-capture process, of stellar nucleosynthesis is called for to
explain the production of the stable (and some long-lived radioactive) neutron-rich nuclides …

Use of the code NuShellX@ MSU is outlined. It connects to the ENSDF data files for
automatic comparisons to energy level data. Operator overlaps provide predictions for …

We propose a thick-restart block Lanczos method, which is an extension of the thick-restart
Lanczos method with the block algorithm, as an eigensolver of the large-scale shell-model …

Motivated by limitations of the Bloch–Horowitz–Brandow perturbative approach to nuclear
structure we have developed the non-perturbative ab initio no core shell model (NCSM) …

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 …

The mass of the nucleus, through its binding energy, continues to be of capital importance
not only for various aspects of nuclear physics, but also for other branches of physics …

The nuclear shell model has perhaps been the most important conceptual and
computational paradigm for the understanding of the structure of atomic nuclei. While the …

The effective interaction GXPF1 for shell-model calculations in the full pf shell is tested in
detail from various viewpoints such as binding energies, electromagnetic moments and …

The cross section for coherent elastic neutrino-nucleus scattering (CE ν NS) depends on the
response of the target nucleus to the external current, in the Standard Model (SM) mediated …