Browsing by Subject "O-18(ALPHA,GAMMA)NE-22"
Now showing items 1-2 of 2
(2003-05-19)Properties of atomic nuclei important for the prediction of astrophysical reaction rates are reviewed. In the first part, a recent simulation of evolution and nucleosynthesis of stars between 15 and 25 M-circle dot is ...
Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics (2003-05-05)We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion ...
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