In addition to long-lived radioactive nuclei like U and Th isotopes, which have been used to
measure the age of theGalaxy, also radioactive nuclei with half-lives between 0.1 and 100 …

Nuclear weak rates in stellar environments are obtained by taking into account recent
advances in shell-model studies of spin-dependent excitation modes in nuclei including …

We study the neutrino-induced production of nuclides in explosive supernova
nucleosynthesis for progenitor stars with solar metallicity including neutrino-nucleus …

Neutrino interactions with stellar material are widely believed to be fundamental to the
explosion of massive stars. However, this important process has remained difficult to confirm …

Gamow–Teller nuclear matrix elements (NMEs) for pairs of β±↔++ 1 0 ground-state-to-
ground-state transitions, in particular their geometric mean NME Mm, are studied. The …

We investigate the neutrino flavor change effects due to neutrino self-interaction and shock
wave propagation, as well as the matter effects on the neutrino process in core-collapsing …

The vortex photon beam induced nuclear reaction is studied. The interaction formalism of
nuclei with vortex photons is developed and incorporated into the statistical reaction model …

We reinvestigate effects of neutrino oscillations on the production of 7 Li and 11 B in core-
collapse supernovae (SNe). During the propagation of neutrinos from the proto–neutron …

We present a new nucleosynthesis process that may take place on neutron-rich ejecta
experiencing an intensive neutrino flux. The nucleosynthesis proceeds similarly to the …

Niobium-92 is an extinct proton-rich nuclide, which decays to 92 Zr with a half-life of 37 Ma.
This radionuclide potentially offers a unique opportunity to determine the timescales of early …