出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：We have calculated r-process nucleosynthesis in a new supernova model, which is driven by
acoustic power generated in the inner core. In our results, plenty of actinide and the third peak
elements are generated. However, light r-process elements around the first and second peak are
overproduced. Our present results indicate that further studies of the r-process in this model are
desirable.
