Direct measurements of (p,γ) cross-sections at astrophysical energies using radioactive beams and the Daresbury Recoil Separator

被引:0
作者
Bardayan, D. W. [1 ]
Chipps, K. A. [2 ]
Fitzgerald, R. P. [3 ]
Blackmon, J. C. [1 ,4 ]
Chae, K. Y. [5 ]
Champagne, A. E. [3 ]
Greife, U. [2 ]
Hatarik, R. [6 ]
Kozub, R. L. [7 ]
Matei, C. [8 ]
Moazen, B. H. [5 ]
Nesaraja, C. D. [1 ]
Pain, S. D. [1 ,6 ]
Peters, W. A. [6 ]
Pittman, S. T. [5 ]
Shriner, J. F., Jr. [7 ]
Smith, M. S. [1 ]
机构
[1] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[2] Colorado Sch Mines, Dept Phys, Golden, CO 80401 USA
[3] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
[4] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[5] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[6] Rutgers State Univ, Dept Phys & Astron, New Brunswick, NJ 08903 USA
[7] Tennessee Technol Univ, Dept Phys, Cookeville, TN 38505 USA
[8] Oak Ridge Associated Univ, Oak Ridge, TN 37830 USA
基金
美国国家科学基金会;
关键词
NUCLEOSYNTHESIS; HRIBF;
D O I
10.1140/epja/i2008-10737-8
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
There are a number of astrophysical environments in which the path of nucleosynthesis proceeds through proton-rich nuclei. These nuclei have traditionally not been available as beams, and thus proton-capture reactions on these nuclei could only be studied indirectly. At the Holifield Radioactive Ion Beam Facility (HRIBF), some of the first direct measurements of (p,gamma) cross-sections on radioactive beams have been made. The Daresbury Recoil Separator (DRS) has been used to separate the recoils of interest from the unreacted primary beam and identify them in an isobutane-filled ionization counter. First data from (17)F(p,gamma) (18)Ne and (7)Be(p,gamma)(8)B measurements are presented.
引用
收藏
页码:457 / 460
页数:4
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