Microscopic methods and tools to describe nuclear dynamics have considerably been
improved in the past few years. They are based on the time-dependent Hartree–Fock …

Now 50 years since the existence of the neutron star crust was proposed, we review the
current understanding of the nuclear physics of the outer layers of accreting neutron stars …

Multinucleon transfer processes in low-energy heavy ion reactions have attracted increasing
interest in recent years aiming at the production of new neutron-rich isotopes. Clearly, it is an …

Above-barrier fusion cross sections for an isotopic chain of oxygen isotopes with A= 16–19
incident on a C 12 target are presented. Experimental data are compared with both static …

The design, construction, and characterization of the Multi-Sampling Ionization Chamber,
MuSIC@ Indiana, are described. This detector provides efficient and accurate measurement …

Fusion excitation functions at energies above the fusion barrier for 12− 15 C+ 12 C are
examined. From these excitation functions the average fusion cross-section,< σ F>, is …

The dynamics of neutron-rich light-mass compound nuclei Mg* 24, 25, 26, 27 formed in C
12, 13, 14, 15+ C 12 fusion reactions, respectively, is explored at different E cm values within …

Stellar nuclear fusion reactions take place in a hot, dense plasma within stars. To account for
the effect of these environments, the theory of open quantum systems is used to conduct …

Systematic examination of fusion for 39, 41, 45, 47 K+ Si 28 and Ar 36, 44+ Si 28 provides
insight into the impact of neutron and proton exchange on fusion for nuclei at and near the …

Fusion enhancement for neutron-rich isotopes of oxygen on carbon nuclei was probed. To
measure the fusion cross section a O 20 beam accelerated to E lab/A= 2.7 MeV bombarded …