出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：Nucleosynthesis in early proton-rich neutrino winds is investigated. The inclusion of
charged-current neutrino reactions on free nucleons indicates that in conditions extracted from a current
supernova model nucleosynthesis will proceed some 40 mass units higher than if they are neglected. An
analytical estimate of how high in Z the nucleosynthesis might proceed as a function of the neutrino flux
and the usual parameters defining the expansion (entropy, Ye, expansion timescale) is presented as well as
the sensitivity of the nucleosynthesis to variations in late time neutron addition and increases to the
entropy predicted in the model due to various physical processes that were not included.
