Speaker
Youngman KIM
(CENS, IBS)
Description
We study the sensitivity of the r-process nucleosynthesis to the nuclear reactions of light nuclei.
We first update nuclear reaction data in Libnucnet code if available in experiments. We then calculate the r-process nucleosynthesis in the core-collapse supernovae and collapsar. For core-collapse supernovae we consider two different scenarios: the magnetohydrodynamic (MHD) jet model and a simple exponential model for the weak r-process.
We find important reactions such as 14C(n, gamma)15C to which the r-process is sensitive. We finally discuss reaction network flows under the various conditions.
Primary authors
Kyungil KIM
(IRIS, IBS)
Motohiko KUSAKABE
(Beihang Univ.)
Shota SHIBAGAKI
(Univ. of Wroclaw)
Toshitaka KAJINO
(Beihang Univ./NAOJ/Univ. of Tokyo)
Xingqun YAO
(Beihang Univ.)
Youngman KIM
(CENS, IBS)
Zhenyu HE
(Beihang Univ.)
