Astrophysical S factor and reaction rate of 92,94Mo(p, γ) relevant to the p-process
Abstract. Low energy proton capture cross sections on heavy isotopes are necessary for a better understanding of the astrophysical p-process. There are around 35 proton-rich stable isotopes between 74S e and 196Hg which are bypassed by the s- and r- processes. These are commonly referred as p-nuclei...
| Published in: | EPJ Web of Conferences |
|---|---|
| Main Authors: | , , , , |
| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2023-01-01
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| Online Access: | https://www.epj-conferences.org/articles/epjconf/pdf/2023/01/epjconf_enas112023_02006.pdf |