“…Nevertheless, their origin has long been discussed with many possible nuclear reactions, and their astrophysical sites have not been identified uniquely. The proposed nuclear processes are the rapid proton capture reactions in novae and type-I X-ray bursts in neutron stars (rp-process) [5,6], the proton-induced reactions by galactic cosmic rays [7], the photodisintegration reactions in supernova (SN) explosions (γ-process or p-process) [4,8,9,10,11,12], and the neutrino-induced reactions in SN explosions (ν-process) [13,14]. The origin of the p-nuclei is crucial to our understanding of how the Solar System material formed and evolved.…”