Investigation of the thermonuclear Ne-18(alpha,p)Na-21 reaction rate via resonant elastic scattering of Na-21 + p | |
Zhang, LY ; He, JJ ; Parikh, A ; Xu, SW ; Yamaguchi, H ; Kahl, D ; Kubono, S ; Mohr, P ; Hu, J ; Ma, P ; Chen, SZ ; Wakabayashi, Y ; Wang, HW ; Tian, WD ; Chen, RF ; Guo, B ; Hashimoto, T ; Togano, Y ; Hayakawa, S ; Teranishi, T ; Iwasa, N ; Yamada, T ; Komatsubara, T ; Zhang, YH ; Zhou, XH | |
刊名 | PHYSICAL REVIEW C |
2014 | |
卷号 | 89期号:1 |
关键词 | ASTROPHYSICAL REACTION-RATES X-RAY-BURSTS SEPARATOR CRIB RP-PROCESS NUCLEOSYNTHESIS STATES BEAM TARGET |
ISSN号 | 0556-2813 |
通讯作者 | jianjunhe@impcas.ac.cn |
英文摘要 | The Ne-18(alpha,p)Na-21 reaction is thought to be one of the key breakout reactions from the hot CNO cycles to the rp process in type I x-ray bursts. In this work, the resonant properties of the compound nucleus Mg-22 have been investigated by measuring the resonant elastic scattering of Na-21 + p. An 89-MeV Na-21 radioactive beam delivered from the CNS Radioactive Ion Beam Separator bombarded an 8.8 mg/cm(2) thick polyethylene (CH2)(n) target. The Na-21 beam intensity was about 2 x 10(5) pps, with a purity of about 70% on target. The recoiled protons were measured at the center-of-mass scattering angles of theta(c.m) approximate to 175.2 degrees, 152.2 degrees, and 150.5 degrees. by three sets of Delta E-E telescopes, respectively. The excitation function was obtained with the thick-target method over energies E-x (Mg-22) = 5.5-9.2 MeV. In total, 23 states above the proton-threshold in Mg-22 were observed, and their resonant parameters were determined via an R-matrix analysis of the excitation functions. We have made several new J(pi) assignments and confirmed some tentative assignments made in previous work. The thermonuclear Ne-18(alpha, p)Na-21 rate has been recalculated based on our recommended spin-parity assignments. The astrophysical impact of our new rate has been investigated through one-zone postprocessing x-ray burst calculations. We find that the Ne-18(alpha, p)Na-21 rate significantly affects the peak nuclear energy generation rate, reaction fluxes, and onset temperature of this breakout reaction in these astrophysical phenomena. |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000332157000004 |
公开日期 | 2015-03-13 |
内容类型 | 期刊论文 |
源URL | [http://ir.sinap.ac.cn/handle/331007/14205] |
专题 | 上海应用物理研究所_中科院上海应用物理研究所2011-2017年 |
推荐引用方式 GB/T 7714 | Zhang, LY,He, JJ,Parikh, A,et al. Investigation of the thermonuclear Ne-18(alpha,p)Na-21 reaction rate via resonant elastic scattering of Na-21 + p[J]. PHYSICAL REVIEW C,2014,89(1). |
APA | Zhang, LY.,He, JJ.,Parikh, A.,Xu, SW.,Yamaguchi, H.,...&Zhou, XH.(2014).Investigation of the thermonuclear Ne-18(alpha,p)Na-21 reaction rate via resonant elastic scattering of Na-21 + p.PHYSICAL REVIEW C,89(1). |
MLA | Zhang, LY,et al."Investigation of the thermonuclear Ne-18(alpha,p)Na-21 reaction rate via resonant elastic scattering of Na-21 + p".PHYSICAL REVIEW C 89.1(2014). |
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