Neutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process
  We present a new nucleosynthesis process, that we denote nu p-process, which occurs in supernovae (and possibly gamma-ray bursts) when strong neutrino fluxes create proton-rich ejecta. In this process, antineutrino absorptions in the proton-rich environment produce neutrons that are immediately captured by neutron-deficient nuclei. This allows for the nucleosynthesis of nuclei with mass numbers A >64. Making this process a possible candidate to explain the origin of the solar abundances of 92,94Mo and 96,98Ru. This process also offers a natural explanation for the large abundance of Sr seen in an hyper-metal-poor star. 
C. Fr\"ohlich, G. Mart\'inez-Pinedo, M. Liebend\"orfer, F.-K.   Thielemann, E. Bravo, W. R. Hix, K. Langanke, and N. T. Zinner