r-process Nucleosynthesis in Supernovae

Kaori Otsuki
2009 Proceedings of 10th Symposium on Nuclei in the Cosmos — PoS(NIC X)   unpublished
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. 10th Symposium on Nuclei in the Cosmos
doi:10.22323/1.053.0141 fatcat:7v4d63twwjdcjokooa4s3wfsea