New measurement of the α asymptotic normalization coefficient of the 1/2+ state in 17O at 6.356 MeV that dominates the 13C(α, n)16O reaction rate at temperatures relevant for the s process

被引:35
作者
Avila, M. L. [1 ]
Rogachev, G. V. [2 ,3 ]
Koshchiy, E. [2 ,3 ]
Baby, L. T. [1 ]
Belarge, J. [1 ]
Kemper, K. W. [1 ]
Kuchera, A. N. [1 ]
Santiago-Gonzalez, D. [1 ]
机构
[1] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA
[2] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA
[3] Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
来源
PHYSICAL REVIEW C | 2015年 / 91卷 / 04期
基金
美国国家科学基金会;
关键词
STARS;
D O I
10.1103/PhysRevC.91.048801
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
Background: Accurate knowledge of the C-13(alpha, n)O-16 reaction cross section is important for the understanding of the s process in asymptotic giant branch stars, since it is considered to be the main source of neutrons. The subthreshold 1/2(+) state at excitation energy of 6.356 MeV in O-17 has a strong influence on the reaction cross section at energies relevant for astrophysics. Several experiments have been performed to determine the contribution of this state to the C-13(alpha, n)(16)Oreaction rate. Nevertheless, significant discrepancies between different measurements remain. Purpose: The aim of this work is to investigate these discrepancies. Method: An 8 MeV 13C beam (below the Coulomb barrier) was used to study the alpha-transfer reaction Li-6(C-13, d)O-17. Results: The squared Coulomb-modified asymptotic normalization coefficient of the 1/2+ state in 17O measured in this work is ((C) over tildeC(alpha-13C)(17O(1/2+)) = 3.6 +/- 0.7 fm(-1). Conclusions: Discrepancy between the results of a-transfer experiments have been resolved. However, some discrepancy with the most recent measurement using the Trojan Horse method remains.
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页数:4
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