975 resultados para F-17


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在兰州放射性束流线(RIBLL)上完成了17F/17O+208Pb的弹性散射微分截面角分布测量.分析了17F/17O弹性散射产物微分截面的对数(ln(dσ/dθ))随散射角平方(θ2)的依赖关系.结果表明,在所测量的角度范围内(6°-20°),17O的这一依赖关系可以用一条直线很好地拟合,而17F的这一依赖关系需要两条不同斜率的直线才能拟合.17F数据拟合中的这种斜率改变可能起因于17F的奇异结构.对其他实验组数据的分析支持以上的结论,即在一定的角度范围内,弱束缚核与稳定核相比,弹性散射产物微分截面的对数与散射角平方的依赖关系有明显的差异,这可以作为深入研究“晕核”和“皮核”的一个新探针.

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描述了在兰州放射性次级束流线上用 80MeV/u的2 0 Ne轰击Be靶产生出理论上预言有奇异结构的17Ne的次级束流 ,并用它轰击Si靶 ,测量它的反应总截面并与其相邻的核相比较 ,发现截面值没有增大的现象 .利用微观的Glauber模型进行了计算 ,理论计算和实验结果符合很好 ,确认其没有奇异结构 .

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观测了低速 (小于Bohr速度 )高电荷Ar17+离子与金属Mo表面相互作用的X射线发射 ,以及ArKα ,KβX射线强度随入射离子动能的变化 .

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在 3 3 .4MeV/u17N束轰击197Au靶产生的反应中 ,利用放置于不同角度组合的 1 7个中子探测器 ( 4°— 83°)和 1 4个半导体望远镜 ( 2 .3°— 9.0°)对反应产物碎片与中子进行了符合测量 .经对所得实验角分布积分得到Z =3— 6元素的同位素产额分布 .在参加者 -旁观者模型框架下 ,采用17N原子核内部的不同密度分布计算了同位素产额分布并与实验数据做比较

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采用逆运动学方法对放射性核束17F和18Ne与质子进行弹性散射实验 ,得到了实验测量微分截面 .用较准确描述放射性核素性质的CH89参数化的光学势为初始光学势 ,用扭曲波玻恩近似的理论计算程序DWUCK4和自动参数搜索程序ABOD对实验数据进行光学势参数理论拟合 ,得到了与实验数据相符合的光学势参数 .将得到的光学势参数进行分析 ,得到了17F和18Ne实势相互作用均方根半径分别为 3 2 3 9fm和 3 3 1 7fm .

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利用HIRFL(兰州重离子研究装置 )产生的 5 5MeV/u的4 0 Ar17+ 离子束 ,在辐照生物学实验终端 ,测量了其经过 1.5mm厚有机玻璃后三个不同角度的碎片分布情况。探索了应用由CsI(Tl) +快塑料闪烁探测器组成的Phoswich探测器研究重离子在生物材料中产生的核碎片角分布测量的可行性 ,结果表明这种实验方法是可行的 ,实验结果令人鼓舞。本工作为进一步的实验积累了可靠的经验。

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应用透射法对中能区F同位素与C靶的反应总截面进行了测量 .发现17F的反应总截面比其邻近同位素的反应总截面稍有增强 .用Glauber模型和BUU模型对F同位素进行了差异因子d的分析 .17F的差异因子d比其附近同位素稍有增强 .分析结果表明17F可能存在质子皮结构 .

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利用RIBLL提供的丰中子放射性束测量了17N在197Au和9Be靶上的破裂反应 .用 1 4单元阵列探测器测量得到了前角带电粒子产额和关联粒子对的破裂截面 ,得到了17N在197Au和9Be靶上的带电粒子破裂截面比为 4— 5倍 ,结果表明对重靶核除了核破裂机制外还要考虑库仑破裂的贡献

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在不同角度测得的 33 4MeV/u17N +9Be反应中 ,发射中子的能谱具有复杂的形式 ,而且随着角度的增大显示出有规律的变化 发射中子至少来源于靶弹核间的核子 -核子碰撞、17N的破裂反应以及熔合热核的统计蒸发三种不同起源 分析结果表明 :反应体系三种起源的发射中子截面分别为 4 4 9,0 4 4和 5 5b

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A measurement of the inelastic component of the key astrophysical resonance in the 14O(α,p)17F reaction for burning and breakout from hot carbon-nitrogen-oxygen (CNO) cycles is reported. The inelastic component is found to be comparable to the ground-state branch and will enhance the 14O(α,p)17F reaction rate. The current results for the reaction rate confirm that the 14O(α,p)17F reaction is unlikely to contribute substantially to burning and breakout from the CNO cycles under novae conditions. The reaction can, however, contribute strongly to the breakout from the hot CNO cycles under the more extreme conditions found in x-ray bursters.

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The total reaction cross section (1724 +/- 93 mb) of B-17 at the energy of 43.7 A MeV on C target has been measured by using the transmission method at the Radioactive Ion Beam Line in Lanzhou (RIBLL). Assuming B-17 consists of a core B-15 plus two halo neutrons, the total cross section of B-17 on C target was calculated with the zero-range Glauber model, where double Gaussian density distributions and Gaussian plus HO density distributions were used. It can fit the experimental data very well. The characteristic of halo structure for B-17 was found with a large diffusion of the neutrons density distribution.

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The reaction cross section of B-17 on C-12 target at (43.7 +/- 2.4) MeV/u has been measured at the Radioactive Ion Beam Line in Lanzhou (RIBLL). The root-mean-square matter radius (R-rms) was deduced to be (2.92 +/- 0.10) fm, while the R-rms of the core and the valence neutron distribution are 2.28 fm and 5.98 fm respectively. Assuming a "core plus 2n" structure in B-17, the mixed configuration of (2s(1/2)) and (1d(5/2)) of the valence neutrons is studied and the s-wave spectroscopic factor is found to be (80 +/- 21)%.

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The differential cross-sections for elastic scattering of F-17 and O-17 on Pb-208 have been measured at Radioactive Ion Beam Line at Lanzhou (RIBLL). The variation of the logarithms of differential cross-sections with the square of scattering angles, viz. angulax dispersion plot, shows clearly that there exists a turning point in the range of small scattering angles (6 degrees-20 degrees) for F-17 due to its exotic structure, while no turning point was observed for O-17. The experimental results have been compared with previous data of other groups. Systematical analysis on the available data seems to conclude that there is an exotic behavior of elastic scattering angular dispersion of weakly bound nuclei with halo or skin structure as compared with that of the stable nuclei. Therefore the fact that the turning point of the elastic scattering angular dispersion plot appears at small angle for weakly bound nuclei can be used as a new probe to investigate the halo and skin phenomenon.