Study of proton resonances in 18Ne via resonant elastic scattering of 17F + p and its astrophysical implication in the stellar reaction of 14O(α, p)17F

被引:23
作者
He, J. J. [1 ]
Hu, J. [1 ,2 ]
Xu, S. W. [1 ]
Chen, Z. Q. [1 ]
Zhang, X. Y. [1 ]
Wang, J. S. [1 ]
Wang, H. W. [3 ]
Tian, W. D. [3 ]
Yu, X. Q. [1 ]
Zhang, L. Y. [1 ,2 ]
Li, L. [1 ,2 ]
Yang, Y. Y. [1 ,2 ]
Ma, P. [1 ]
Zhang, X. H. [1 ]
Su, J. [4 ]
Li, E. T. [4 ]
Hu, Z. G. [1 ]
Guo, Z. Y. [1 ]
Xu, X. [1 ,2 ]
Yuan, X. H. [1 ]
Lu, W. [1 ,2 ]
Yu, Y. H. [1 ]
Zang, Y. D. [1 ,2 ]
Ye, S. W. [1 ,2 ]
Ye, R. P. [1 ,2 ]
Chen, J. D. [1 ,2 ]
Jin, S. L. [1 ,2 ]
Du, C. M. [1 ,2 ]
Wang, S. T. [1 ,2 ]
Ma, J. B. [1 ]
Liu, L. X. [1 ,2 ]
Bai, Z. [1 ,2 ]
Li, X. Q. [5 ,6 ]
Lei, X. G. [1 ]
Sun, Z. Y. [1 ]
Zhang, Y. H. [1 ]
Zhou, X. H. [1 ]
Xu, H. S. [1 ]
机构
[1] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
[2] Chinese Acad Sci, Grad Sch, Beijing 100049, Peoples R China
[3] Chinese Acad Sci, Shanghai Inst Appl Phys SINAP, Shanghai 201800, Peoples R China
[4] China Inst Atom Energy CIAE, Beijing 102413, Peoples R China
[5] Peking Univ, Sch Phys, Beijing 100871, Peoples R China
[6] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
基金
中国国家自然科学基金;
关键词
SHORT-LIVED NUCLEI; STELLAR REACTIONS; NEUTRON-STARS; RP-PROCESS; ALPHA; O-14; NUCLEOSYNTHESIS; LANZHOU; BEAMS;
D O I
10.1140/epja/i2011-11067-6
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
The stellar O-14(alpha, p) F-17 reaction is thought to be one of the most important breakout reactions from the Hot CNO cycles into the rp-process in Type I X-ray bursters. In the present work, the properties of proton resonances in Ne-18 have been investigated efficiently by utilizing a technique of proton resonant elastic scattering with a F-17 radioactive-ion (RI) beam and a thick proton target. A 4.22MeV/nucleon F-17 RI beam, which was produced via a projectile-fragmentation reaction and experiencing a series of energy degradation, was separated by a Radioactive Ion Beam Line in Lanzhou (RIBLL) and bombarded a (CH2)(n) target. Energy spectra of the recoiled protons were measured by two sets of Delta E-E silicon telescope at center-of-mass scattering angles of theta(c.m.) approximate to 175 degrees +/- 5 degrees, theta(c.m.) approximate to 152 degrees +/- 8 degrees, respectively. Several proton resonances in Ne-18 were observed, and their resonant parameters have been determined by an R-matrix analysis of the differential cross-sections. A doublet structure around 7.10MeV has been identified and thought to be one state at 7.05MeV (2(+)) and another one at 7.12MeV (4(+)). The presently calculated total reaction rates of O-14(alpha, p) F-17 are, at least, a factor of 1.2 similar to 1.9 larger than the previous ones in a temperature region of 1.7 similar to 3.0 GK mainly owing to the contribution from the 7.05MeV (2(+)) state. This result implies that this breakout reaction may play a more important role than previously expected.
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页数:8
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