“…Such a competition between photo-proton σ(γ, p) and photo-neutron σ(γ, n) cross sections impacts a variety of nuclear and astrophysics phenomena -namely, bremsstrahlung [3,4], nuclear polarizability [5], threenucleon forces [6], collective properties [7], isospin asymmetry and symmetry energy in neutron stars [8][9][10][11], neon and silicon burning at the end of stellar evolution [12] and the nucleosynthesis of p-nuclei [13,14], which are shielded from the rapid-neutron capture by stable isobars. A recent review article by Zilges and co-workers discusses in detail various applications of photonuclear physics [15], e.g. finding new routes for production of medical radioisotopes or nuclear-waste transmutation.…”