In this Report we give a balanced account of the experimental and theoretical advances
acquired over the last decade in the field of near-barrier fusion reactions induced by weakly …

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 …

The GEF (“GEneral description of Fission observables”) model code is documented. It
describes the observables for spontaneous fission, neutron-induced fission and, more …

The study of fusion reactions at extreme sub-barrier energies has seen an increased interest
in recent years, although difficult to measure due to their very small cross sections. Such …

In the past 85 years the number of known nuclides increased by more than a factor of ten,
resulting in 4000 presently known isotopes of 118 elements. This considerable progress we …

Atomic nuclei are composite systems, and they may be dynamically excited during nuclear
reactions. Such excitations are not only relevant to inelastic scattering but they also affect …

The C 12+ C 12 fusion reaction plays a critical role in the evolution of massive stars and also
strongly impacts various explosive astrophysical scenarios. The presence of resonances in …

We present a microscopic study on the fusion reactions C 14, 15+ Th 232 by emphasizing
the effect of deformed halo structure on reaction dynamics within the framework of time …

Carbon burning is a critical phase for nucleosynthesis in massive stars. The conditions for
igniting this burning stage, and the subsequent isotope composition of the resulting ashes …

The phenomenon of incomplete fusion (ICF) using both the strongly and weakly bound
projectiles below an incident energy of≈ 10 MeV per nucleon is reviewed. Various reaction …