Nucleosynthesis simulations for the production of the p-nuclei $^{\text{92}}$Mo and $^{\text{94}}$Mo in a Supernova type II model
英文摘要：
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.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
