Search
Now showing items 1-2 of 2
Nucleosynthesis in massive stars with improved nuclear and stellar physics
(2002-09-01)
We present the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in stellar models computed from the onset of central hydrogen burning through explosion as Type II supernovae. ...
Massive star evolution : nucleosynthesis and nuclear reaction rate uncertainties
(2002-07)
We present a nucleosynthesis calculation of a 25 M-circle dot star of solar composition that includes all relevant isotopes up to polonium. We follow the stellar evolution from hydrogen burning till iron core collapse and ...