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Examination of the role of the O-14(alpha, p)F-17 reaction rate in type-I x-ray bursts
Hu, J; He, JJ; Parikh, A; Xu, SW; Yamaguchi, H; Kahl, D; Ma, P; Su, J; Wang, HW; Nakao, T; Wakabayashi, Y; Teranishi, T; Hahn, KI; Moon, JY; Jung, HS; Hashimoto, T; Chen, AA; Irvine, D; Lee, CS; Kubono, S; jianjunhe@impcas.ac.cn; anuj.r.parikh@upc.edu
2014
Source PublicationPHYSICAL REVIEW C
ISSN0556-2813
Volume90Issue:2
AbstractThe O-14(alpha, p)F-17 reaction is one of the key reactions involved in the breakout from the hot-CNO cycle to the rp-process in type-I x-ray bursts (XRBs). The resonant properties in the compound nucleus Ne-18 have been investigated through resonant elastic scattering of F-17 + p. The radioactive F-17 beam was separated by the Center for Nuclear Study radioactive ion beam separator (CRIB) and bombarded a thick H-2 gas target at 3.6 MeV/nucleon. The recoiling light particles were measured by three Delta E-E silicon telescopes at laboratory angles of theta(lab) approximate to 3 degrees, 10 degrees, and 18 degrees. Five resonances at E-x = 6.15, 6.28, 6.35, 6.85, and 7.05 MeV were observed in the excitation functions, and their spin-parities have been determined based on an R-matrix analysis. In particular, J(pi) = 1(-) was firmly assigned to the 6.15-MeV state which dominates the thermonuclear O-14(alpha, p)F-17 rate below 2 GK. As well, a possible new excited state in Ne-18 was observed at E-x = 6.85 +/- 0.11 MeV with tentative J = 0 assignment. This state could be the analog state of the 6.880 MeV (0(-)) level in the mirror nucleus O-18, or a bandhead state (0(+)) of the six-particle four-hole (6p-4h) band. A new thermonuclear O-14(alpha, p)F-17 rate has been determined, and the astrophysical impact of multiple recent rates has been examined using an XRB model. Contrary to previous expectations, we find only a modest impact on predicted nuclear energy generation rates from using reaction rates differing by up to several orders of magnitude.
KeywordAstrophysical Reaction-rates Accreting Neutron-stars Short-lived Nuclei Hot Cno Cycle Resonance Scattering Elastic-scattering Stellar Reactions Separator Crib Rp-process Nucleosynthesis
Indexed BySCI
Language英语
WOS IDWOS:000341240300005
Citation statistics
Cited Times:14[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/14127
Collection中科院上海应用物理研究所2011-2019年
Corresponding Authorjianjunhe@impcas.ac.cn; anuj.r.parikh@upc.edu
Recommended Citation
GB/T 7714
Hu, J,He, JJ,Parikh, A,et al. Examination of the role of the O-14(alpha, p)F-17 reaction rate in type-I x-ray bursts[J]. PHYSICAL REVIEW C,2014,90(2).
APA Hu, J.,He, JJ.,Parikh, A.,Xu, SW.,Yamaguchi, H.,...&anuj.r.parikh@upc.edu.(2014).Examination of the role of the O-14(alpha, p)F-17 reaction rate in type-I x-ray bursts.PHYSICAL REVIEW C,90(2).
MLA Hu, J,et al."Examination of the role of the O-14(alpha, p)F-17 reaction rate in type-I x-ray bursts".PHYSICAL REVIEW C 90.2(2014).
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