Scaling relations for the supernova γ-process and the 176Lu nuclear cosmochronometer

被引:8
作者
Hayakawa, T [1 ]
Iwamoto, N
Shizuma, T
Kajino, T
Umeda, H
Nomoto, K
机构
[1] Japan Atom Energy Res Inst, Adv Photon Res Ctr, Kyoto 6190215, Japan
[2] Natl Astron Observat, Mitaka, Tokyo 1818588, Japan
[3] Japan Atom Energy Res Inst, Dept Nucl Energy Syst, Tokai, Ibaraki 3191195, Japan
[4] Univ Tokyo, Sch Sci, Dept Astron, Tokyo 1130033, Japan
关键词
D O I
10.1016/j.nuclphysa.2005.05.095
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Analyzing the solar system abundances, we find two universal scaling relations concerning the p- and s-nuclei. These scalings indicate that the gamma-process nucleosynthesis in supernova, (SN) explosions is the most probable origin of the p-nuclei. In addition the scalings lead to new concepts: a universality of the gamma-process and a new nuclear cosmochronometer. Calculations of the gamma-process are carried out for typical core-collapse SN explosion models. These confirm the observed
引用
收藏
页码:525C / 528C
页数:4
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