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Excited States in 18Ne Studied via 17F+p * |
JIN Sun-Jun1, 2, WANG You-Bao1, WANG Bao-Xiang1, BAI Xi-Xiang1, FANG Xiao1, GUO Bing1, LI Er-Tao1, LI Yun-Ju1, LI Zhi-Hong1, LIAN Gang1, SU Jun1, YAN Sheng-Quan1, ZENG Sheng1, YAO Ze-En2, LIU Wei-Ping1
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| 1China Institute of Atomic Energy, PO Box 275(46), Beijing 102413 2School of Nuclear Science and Technology, Lanzhou University, Lanzhou 730000 |
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| Cite this article: |
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JIN Sun-Jun, WANG You-Bao, WANG Bao-Xiang et al 2010 Chin. Phys. Lett. 27 032102 |
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Abstract The elastic resonance scattering of 17F+p is studied in inverse kinematics via a thick-target method. The excitation function for 17F+p elastic scattering is obtained within the energy interval of Ec.m ≈ 0.4-1.7 MeV. The experimental excitation function is analyzed with a multilevel R-matrix code MULTI7, and the proton widths are deduced. The α decay from 6.15 MeV 1- state in 18Ne is observed, which is critical to the 14O(α, p)17F reaction as the main breakout route from CNO cycle to rp-process in supernovae and x-ray bursts.
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| Keywords:
21.10.HW
21.10.Jx
25.40.Ny
27.20.+n
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Received: 15 November 2009
Published: 09 March 2010
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| PACS: |
21.10.Hw
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(Spin, parity, and isobaric spin)
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21.10.Jx
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(Spectroscopic factors and asymptotic normalization coefficients)
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25.40.Ny
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(Resonance reactions)
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27.20.+n
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(6 ≤ A ≤ 19)
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[1] Wallerstein G 1997 Rev. Mod. Phys. 69 995
[2] Schatz H et al 1998 Phys. Rep. 294 167
[3] Burbidge E M et al 1957 Rev. Mod. Phys. 29 547
[4] Wiescher M, G\"{orres J and Schatz H 1999 J. Phys. G 25 R133
[5] Wallace R K and Woosley S E 1981 Astrophys. J. Suppl. 45 389
[6] Bardayan D W et al 1999 Phys. Rev. Lett. 83 45
[7] G\'{omez del Campo J et al 2001 Phys. Rev. Lett. 86 43
[8] Harss B et al 1999 Phys. Rev. Lett. 82 3964
[9] Harss B et al 2002 Phys. Rev. C 65 035803
[10] Blackmon J C et al 2001 Nucl. Phys. A 688 142c
[11] Blackmon J C et al 2003 Nucl. Phys. A 718 127c
[12] Wang Y B et al 2006 High Energy Phys. Nucl. Phys. (suppl. I$\!$I) 30 202 (in Chinese)
[13] Wang Y B et al 2008 Phys. Rev. C 77 044304
[14] Qin X et al 2008 Chin. Phys. C 32 957
[15] Wang Y B et al 2009 Chin. Phys. C 33 181
[16] Artemov K P et al 1990 Sov. J. Nucl. Phys. 52 408
[17] Smith M S and Rehm K E 2001 Annu. Rev. Nucl. Part. Sci. 51 91
[18] Markenroth K et al 2000 Phys. Rev. C~ 62 034308
[19] Teranishi T et al 2003 Phys. Lett. B 556 27
[20] Ruiz C et al 2005 Phys. Rev. C 71 025802
[21] He J J et al 2009 Phys. Rev. C 80 015801 |
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