Searching for (γ, α)/(γ, n) branching points in the γ-process path near A=100

被引:6
|
作者
Kelmar, R. [1 ,2 ]
Simon, A. [1 ,2 ]
Olivas-Gomez, O. [1 ,2 ]
Millican, P. [1 ,2 ]
Reingold, C. S. [1 ,2 ]
Churchman, E. [1 ,2 ]
Clark, A. M. [1 ,2 ]
Henderson, S. L. [1 ,2 ]
Kelly, S. E. [1 ,2 ]
Robertson, D. [1 ,2 ]
Stech, E. [1 ,2 ]
Tan, W. P. [1 ,2 ]
机构
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[2] Univ Notre Dame, Joint Inst Nucl Astrophys, Notre Dame, IN 46556 USA
基金
美国国家科学基金会;
关键词
ASTROPHYSICAL REACTION-RATES; MODEL; DENSITY; POTENTIALS;
D O I
10.1103/PhysRevC.101.015801
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
Four (alpha, gamma) cross-section measurements on stable nuclei in the A = 100 mass range were performed at the University of Notre Dame Nuclear Science Laboratory. The Pd-102(alpha, gamma)Cd-106 and Cd-110(alpha, gamma)Sn-114 reactions were measured for the first time. The Zr-90(alpha, gamma)Mo-94 and Cd-108(alpha, gamma)Sn-112 results extended the measured range down to energies lower than those of the previous experiments. These reactions were studied as possible branching points in gamma-process reaction networks. The measured cross-section values were compared to the NONSMOKER database as well as to calculations performed with TALYS 1.9. The combination of parameters available in TALYS that gave the best fit to the data was found and the corresponding reaction rates were obtained. The inverse (gamma, alpha) rates were then obtained and compared to the corresponding (gamma, n) rates to investigate the relative strength between the two reaction pathways. It was found that in all four cases the (gamma, alpha) reaction pathway begins to dominate within the 1.5-3.5 GK temperature range.
引用
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页数:9
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