Abstract
We investigate the r-process that occurs due to the explosion from an inner region of the Fe-core. It is shown that the solar r-process abundances are rather well reproduced for a model of 13 M⊙. We also examine whether the fission affects final r-process abundances by using the full nuclear reaction network with both spontaneous and the β-delayed fission included. Moreover, we pay attention how the mass formula affects the r-process peaks by using two networks.
Original language | English |
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Pages (from-to) | 635-638 |
Number of pages | 4 |
Journal | Nuclear Physics A |
Volume | 758 |
Issue number | 1-4 SPEC. ISS. |
DOIs | |
Publication status | Published - Jul 25 2005 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics