Nucleosynthesis simulations for the production of the p-nuclei 92Mo and 94Mo in a Supernova type II model

We present a nucleosynthesis sensitivity study for the γ -process in a Supernova type II model within the NuGrid research platform. The simulations aimed at identifying the relevant local production and destruction rates for the p-nuclei of molybdenum and at determining the sensitivity of the final abundances to these rates. We show that local destruction rates strongly determine the abundance of 92 Mo and 94 Mo, and quantify the impact