17O(α,γ)21Ne and 17O(α,n)20Ne for the weak s process

被引:0
|
作者
Best, A. [1 ]
Goerres, J. [1 ]
Beard, M. [1 ]
Couder, M. [1 ]
deBoer, R. [1 ]
Falahat, S. [1 ,2 ]
Gueray, R. T. [3 ]
Kontos, A. [1 ]
Kratz, K-L [2 ]
LeBlanc, P. J. [1 ]
Li, Q. [1 ]
O'Brien, S. [1 ]
Oezkan, N. [3 ]
Pignatari, M. [4 ]
Sonnabend, K. [5 ]
Talwar, R. [1 ]
Tan, W. [1 ]
Uberseder, E. [1 ]
Wiescher, M. [1 ]
机构
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[2] Kacaeli Univ, Dept Phys, D-55020 Mainz, Germany
[3] Kacaeli Univ, Dept Phys, TR-41380 Umuttepe, Turkey
[4] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
[5] Goethe Univ Frankfurt, Inst Appl Phys, D-60325 Frankfurt, Germany
基金
美国国家科学基金会;
关键词
Helium burning; neutron poison; s process; R matrix; PROCESS NUCLEOSYNTHESIS; NE-21;
D O I
10.1063/1.4768509
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ratio of the reaction rates of the competing channels O-17(alpha,gamma)Ne-21 and O-17(alpha,n)Ne-20 determines the efficiency of O-16 as a neutron poison in the s process in low metallicity rotating stars. It has a large impact on the element production, either producing elements to the mass range of A=90 in case of a significant poisoning effect or extending the mass range up to the region of A=150 if the gamma channel is of negligible strength. We present an improved study of the reaction O-17(alpha, n)Ne-20, including an independent measurement of the O-17(alpha, n(1))Ne-20 channel. A simultaneous R-Matrix fit to both the n(0) and the n(1) channels has been performed. New reaction rates, including recent data on the O-17(alpha,gamma)Ne-21 reaction, have been calculated and used as input for stellar network calculations and their impact on the s process in rotating massive stars is discussed.
引用
收藏
页码:309 / 313
页数:5
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