Determining the 14O(α,p)17F astrophysical rate from Measurements at TwinSol

被引:0
作者
Bardayan, D. W. [1 ]
Ahn, T. [1 ]
Allen, J. M. [1 ]
Brodeur, M. [1 ]
Frentz, B. [1 ]
Gupta, Y. K. [1 ]
Hall, M. R. [1 ]
Hall, O. [1 ]
Henderson, S. [1 ]
Hu, J. [1 ]
Kelly, J. M. [1 ]
Kolata, J. J. [1 ]
Long, A. [1 ]
Nicoloff, C. [1 ]
O'Malley, P. D. [1 ]
Ostdiek, K. [1 ]
Smith, M. K. [1 ]
Strauss, S. [1 ]
Becchetti, F. D. [2 ]
Riggins, J. [2 ]
Torres-Isea, R. O. [2 ]
Blackmon, J. C. [3 ]
Macon, K. [3 ]
Chipps, K. A. [4 ]
Pain, S. D. [4 ]
Rogers, A. M. [5 ]
机构
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[2] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[3] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[4] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[5] Univ Massachusetts, Dept Phys, Lowell, MA 01854 USA
来源
CONFERENCE ON THE APPLICATION OF ACCELERATORS IN RESEARCH AND INDUSTRY (CAARI 2016) | 2017年 / 90卷
基金
美国国家科学基金会;
关键词
nucleosynthesis; radioactive; X-ray; astrophysical;
D O I
10.1016/j.phpro.2017.09.043
中图分类号
T [工业技术];
学科分类号
08 ;
摘要
The O-14(alpha,p)F-17 reaction is an important trigger reaction to the alpha-p process in X-ray bursts. The most stringent experimental constraints on its astrophysical rate come from measurements of the time-inverse reaction, F-17(p,alpha)O-14. Previous studies of this inverse reaction have sufficiently characterized the high-energy dependence of the cross section but there are still significant uncertainties at lower energies. A new measurement of the F-17(p,alpha)O-14 cross section is underway at the Twin Solenoid (TwinSol) facility at the University of Notre Dame using an in-flight secondary F-17 beam. The initial results are promising but improvements are needed to complete the measurement. The initial data and plans for an improved measurement are presented in this manuscript. (C) 2017 The Authors. Published by Elsevier B.V.
引用
收藏
页码:415 / 420
页数:6
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