Influence of nuclear reaction rates on the nucleosynthesis in neutrino-driven winds

被引:1
|
作者
Froehlich, Carla [1 ]
Hatcher, Daniel [1 ,2 ]
机构
[1] N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA
[2] Appalachian State Univ, Dept Phys & Astron, Boone, NC 28608 USA
来源
CGS15 - CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS | 2015年 / 93卷
关键词
RP-PROCESS; RATE TABLES; UNCERTAINTIES; EVOLUTION;
D O I
10.1051/epjconf/20159303008
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study the sensitivity of the nu p-process abundance pattern to (n,p), (p,gamma), and (n,gamma) rates for nuclei between Ni and Sn. We illustrate our findings for two different initial electron fractions and a representative trajectory. We discuss how these rates influence the abundance pattern and the nuclear flow.
引用
收藏
页数:5
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