F同位素的反应总截面测量和~(17)F可能的质子皮结构

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 .

~(17)N破裂反应产物的测量

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

在33.4MeV/u~(17)N与~9Be反应中中子发射的起源

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

Measurement of the inelastic branch of the O-14(alpha, p)F-17 reaction: Implications for explosive burning in novae and x-ray bursters

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.

The properties of halo structure for B-17

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.

Configuration of the valence neutrons of B-17

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)%.

Elastic scattering angular dispersion of weakly bound nucleus F-17

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.

Exotic behavior of elastic scattering differential cross-sections of weakly bound nucleus F-17 at small angles

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 shows clearly that there exists a turning point in the range of small scattering angles (6 degrees-20 degrees) for F-17 having exotic structure, while no turning point was observed in the O-17 elastic scattering. The experimental results have been compared with previous data. Systematical analysis on the available data seems to conclude that there is an exotic behavior of elastic scattering differential cross-sections of weakly bound nuclei with halo or skin structure as compared with that of the ordinary nuclei near stable line. Therefore the fact that the turning point of the logarithms of differential cross-sections appears at small angle for weakly bound nuclei could be used as a new probe to investigate the halo and skin phenomenon.

Exotic behaviour of angular dispersion of weakly bound nucleus F-17 at small angles

The differential cross sections of F-17 and O-17 elastic scattering products on Pb-208 have been measured at the Radioactive Ion Beam Line at Lanzhou (RIBLL). Two angular dispersion plots of ln(d sigma/d theta) versus theta 2 are obtained from the angular distribution of the elastic scattering differential cross sections. The angular dispersion plot exhibits a clear turning point for F-17 in the range of small scattering angles 6 degrees-20 degrees due to its exotic structure, but for O-17, the turning point is not observed in the same angular range. The experimental results have been compared with previous data of other groups. Systematical analysis on the available data supports the above conclusion that there is an exotic behaviour of the angular dispersion plot of weakly bound nuclei with halo or skin structure as compared with that of the ordinary nuclei near stable line. Therefore the turning point of the angular dispersion plot appears at small angle for weakly bound nuclei with halo or skin structure, and can be used as a new probe to investigate the halo and skin phenomena of weakly bound nuclei.

低速~(40)Ar~(17+)离子入射金属Be表面发射的近红外光谱线和X射线谱；Infrared Light and X-ray Emissions of ~(40)Ar~(17+) Impacting on Be Surface ；

用速度不同的(动能EK=272和357keV,速度v=1.14×106和1.72×106m/s)的高电荷态离子40Ar17+分别入射金属Be表面,同时测量这种相互作用过程中产生的近红外光谱线和X射线谱。实验结果表明,在低速范围内(速度小于玻尔速度vBohr=2.19×106m/s),速度较小的40Ar17+离子在到达金属的表面临界距离Rc到进入表面(2—3原子层)的进程中,形成了较多的高激发态Ar原子,其退激辐射较强的光谱线,进而验证了经典过垒模型。

Measurement of the inelastic branch of the stellar O-14(alpha,p)F-17 reaction occurring in the explosive burning in Novae and X-ray busters

The inelastic component of the key astrophysical resonance (1(-), E-x=6.15 MeV) in the O-14(alpha,p)F-17 reaction has been studied by using the resonant scattering of F-17+p. The experiment was done at REX-ISOLDE CERN with the Miniball setup. The thick target method in inverse kinematics was utilized in the present experiment where a 44.2 MeV F-17 beam bombarded a similar to 40 mu m thick (CH2)(n) target. The inelastic scattering protons in coincidence with the de-excited 495 keV gamma rays have been clearly seen and they are from the inelastic branch to the first excited state in F-17 following decay of the 1(-) resonance in Ne-18. Some preliminary results are reported.

Experimental study of the two-proton correlated emission from the excited states of Ne-17,Ne-18 and S-28,S-29

A series of experiments have been performed by complete kinematics measurements to study two-proton (2p) correlated emission from the excited states of Ne-17,Ne-18 and S-28,S-29 via the Coulomb excitation by bombarding on Au-197 target. 2p and residua coincident events were picked Out under strict conditions. Visible p-p correlations were observed. It is shown that 2p can be emitted from the high-lying excited states. 2p halo may lead to 2p emission with large spectroscopy factor for the states close to or beyond the threshold.

奇奇核166,168Lu和奇中子核87Zr高自旋态的实验研究

本论文主要进行了奇奇核~(166)Lu、~(168)Lu和奇中子核~(87)Zr的高自旋态的研究工作，对它们高自旋态的一些物理现象进行了讨论。并且首次对1／2~-[541](direct X)vi_(13/2)组态带的系统学规律进行了总结。主要由以下三个部分组成：~(166,168)Lu高自旋态的研究在最近有关形变奇奇核高自旋态的研究工作中，随着实验上π1／2-[541](direct X)vi_(13/2)带自旋的确定，人们发现除了130区的兀h_(11/2)(direct X)vh_(11/2)和160区的兀h_(11/2)(direct X)vi_(13/2)组态带低自旋旋称反转以外，π1／2~-[541](direct X)vi_(13/2)带的低自旋也是反转的，该转动带低自旋旋称反转现象引起了人们的很大的兴趣并得到很广泛的研究，为了通过π1／2~-[541](direct X)vi_(13/2)带与已知自旋和宇称的基态和一些低激发态相连，确定该转动带的自旋，人们付出了很大的努力。特别是最近几年，一些实验上自旋的确定，使得研究π1／2~-[541](direct X)vi_(13/2)组态带低自旋旋称反转的系统学规律成为可能。需要指出的是在以前的研究结果中，~(166)Lu的π1／2~-[541](direct X)vi_(13/2)组态带的能级摆动规律与相邻奇奇核该组态带的能级摆动规律严重不符，澄清该疑点是我们重新研究该核的主要动力之一。在以前~(168)Lu的研究工作中，只在~(168)Lu中发现两个带，但其中只有晕带的组态得到指定，根据带结构和旋称劈裂的大小估计另一个带极有可能是π1／2~-[541](direct X)vi_(13/2)带。为了澄清以上这些疑点和得到π1／2~-[541](direct X)vi_(13/2)组态带的系统学规律，我们重新研究了。~(166,168)Lu的高自旋态。另外(h_(11/2)_p(i_(13/2))_n组．态带的低自旋旋称反转是一个广为人知的物理现象，但在以前的有关~(166）Lu的结果中对(h_(11/2))_p(i_(13/2))_n组态带白旋的确定与该组态带低自旋旋称反转系统规律相反，这也是我们对~(166)Lu重新研究的一个原因。实验是在北京中国原子能科学研究院HI-13串列加速器上进行的，分别利用入射能量为97MeV和92MeV的~(19)F束通过熔合蒸发反应~(152)Sm(~(19)F,~5n)~(166)Lu和~(154)Sm(~(19)F5n)~(168)Lu布居了~(166)Lu和~(168)Lu的高自旋态。用十台HpGe探测器组成的探测阵列进行γ-γ符合测量，对~(166)Lu和~(168)Lu分别记录了约1.27 * 10~8和0.25 * 10~8个两重和两重以上的符合事件。在~(166)Lu中，共发现了五条转动带，根据它们的顺排在0.28MeV均没有出现上弯，意味着它们的中子均占居i_(13/2)轨道，同时根据在~(165)Lu和~(167)Lu只发现基于9／2~-[514]、7／2~-[404]、1／2~-[541]、1／2~+[411]和5／2~+[402]轨道的转动带及在~(165)Yb和~(167)Hf中晕带均为5／2~+[642]的事实，那么由上述质子轨道和中子轨道组成的转动带是本文发现的五条带的最可能的侯选者。本实验中观察到的五条转动带分别基于7／2~+[404](direct X)5／2~+[642]、9／2~-[514](direct X)5／2~+[642]、1／2~-[541](direct X)5／2~+[642]、5／2~+[402](direct X)5／2~+[642]和1／2~+[642](direct X)5／2~+[642]轨道的转动带。和以前的数据相比主要有以下几点改进：(A)在以前的结果中，包括2000年新发表的有关~(166)Lu的文章，他们均把本文~(166)Lu纲图中(5)和(6)退激系列归属于π1／2~-[541](direct X)v5／2~+[642]转动带，而在本文中通过符合关系一个新的退激系列(7)被发现，根据(6)和(7)之间的符合关系、带交叉频率、γ射线强度和B(M1)／B(E2)的比值等关系，本文认为新发现的退激系列(7)与(6)组成新的π1／2~-[541](direct X)v5／2~+[642]转动带.以前的结果的错误在于把属于1／2~-[541](direct X)5／2~+[642]转动带的α = 0与1／2~-[541](direct X)5／2~+[642]转动带的α = 0误归于一个带，这就澄清了原文献中π1／2~-[541](direct X)v5／2~+[642]转动带能级摆动规律与相邻奇奇核该组态带能级摆动规律不符的疑点，同时把原文献中误归于π1／2~-[541](direct X)v5／2~+[642]转动带的那一个退激系列(5)重新指定为1／2~+[411](direct X)5／2~+[642]带(α = 0)；(B)通过分析实验数据、跃迁能量系统学和运用顺排相加性规则对以前实验中建立的9／2~-[514](direct X)5／2~+[642]和7／2~+[404](direct X)5／2~+[642]带的自旋进行了重新指定，把它们的自旋在原文的基础上加1个单位，澄清了以前的有关~(166)Lu结果中对9／2~-[514](direct X)5／2~+[642]组态带自旋的确定与该组态带低自旋旋称反转事实相反的疑点；(C)新发现了基于9／2~-[541](direct X)5／2~+[642]组态的转动带。在~(168)Lu中，共观察到了四条转动带，分别是π1／2~-[541](direct X)v5／2~+[642]、7／2~+[404](direct X)5／2~+[642]、 9／2~-[514](direct X)5／2~+[642]和7／2~+[404](direct X)5/2~-[523](本文新建立的带)带，本文对其中晕带7／2~+[404](direct X)5／2~+[642]的K值取值与原文献中的取值不同，并根据能量系统学和带头激发能指出不同的原因。 除以上所述外，本文还给出了~(166)Lu和~(168)Lu各γ射线的强度、转动参数A、较强γ射线的DCO值、分支比和B(M1)／B(E2)等实验值。基于实验和理论预期的B(M1)／B(E2)比值的比较、各带带交叉行为、顺排相加性、带头激发能和转动参数A对各带的组态和自旋进行了指定。最后通过对实验上对~(162,164)Tm、~(174)Ta和~(176)Re的π1／2~-[541](direct X)vi_(13/2)组态带p-n剩余相互作用信息的提取，指出奇质子核中1／2~-[541]带的带交叉频率相对相邻偶偶核的延迟约三分之一到一半左右，其原因是由于p-n剩余相互作用所造成的(包含了对效应和形变变化的CSM模型能够解释另一半的偏离)，可以定性的认为正是由于形变、对相互作用的变化和剩余p-n相互作用三者相结合导致了整个的1／2~-[541]带中带交叉频率的偏离。旋称反转机制综述和πh_(932)(direct X)vi_(l3/2)组态的系统学首先对导致旋称反转的各种机制做一简单回顾，同时对ππh,u2⑩vi,钔组态带系统学规律做一简单总结，总结了πh_(11/2)(direct X)Vi_(13/2)组态带的跃迁能量系统学规律。在最近，随着~(162)Tm、~(164)Tm、~(174)Ta和~(176)Re等几个奇奇核中半退耦带1／2~-[541](direct X)vi_(13/2)的自旋通过实验方法的确定，人们惊奇的发现在上述这些核~(162)Tm、~(164)Tm、~(174)Ta和~(176)Re)中半退耦带1／2~-[541](direct X)vi_(13/2)在低自旋区都是旋称反转的。人们就会很自然的回头去看那些在该区已经布居1／2~-[541](direct X)vi_(l3／2)组态带的那些核，结果发现对于该组态带的自旋的指定是很杂乱无章的，有些自旋的确定即不符合能量系统学又与顺排相加性规则相悖，如在~(172)Ta和~(178)Re中(值得指出的是有关这两个核的文章均是在十年前发表的)，自旋的指定明显与最近发表的该区πhg_(9/2)(direct X)vi_(13/2)组态带自旋不符，本文通过能量系统学和顺排相加性对~(172)Ta和~(178)Re的1／2~-541](direct X)vi_(13/2)组态带自旋做了修改，分别增加了3h和h。本文通过对最新结果~(162)Tm、~(164)Tm、~(170)Lu、~(170,174,176)Ta、~(176)Re、~(180)Ir)和以前的结果(~(172)Ta和~(178)Re)及本文的结果(~(166,168)Lu)对上述12个核的1／2~-[541](direct X)vi_(13/2)组态带的S(I) = E(I)-E(I-1)- E(I + 2)-E(I + 1)-E(I - 1)-E(I - 2)]／2～I的变化图的分析，继A ≈ 130区7πh_(11/2)(direct X)vh_(11/2)组态带和A ≈ 160区πh_(11/2)(direct X)vi_(13/2)组态带的系统学规律以后，首次总结出A ≈ 170区π1／2~-541](direct X)vi_(13/2)组态带的系统学规律：反转点的自旋随N的增加而增加，随Z的增加而减小，与πh_(11/2)(direct X)和πh_(11/2)(direct X)vi_(13/2)转动带的系统学规律很相似，即反转点自旋均随中子和质子单调地变化。通过对各种理论模型的研究发现三轴形变、科里奥利力、带交叉与自反转和p-n相互作用在奇奇核中都有可能导致旋称反转，包含有p-n相互作用的粒子-转子模型在πh_(11/2)(direct X)和vh_(11/2)、πh_(11/2)和π1／2 ~-[541](direct X)vi_(13/2)组态带中的旋称反转上取得了某些成功，表明p-n相互作用在解释奇核低自旋反转现象中起着很重要的作用。通过对实验上π1／2~-[541](direct X)vi_(13/2)组态带旋称反转点与文献中理论计算值的比较，得出p-n相互作用强度的变化可能是导致π1／2~-[541](direct X)vi_(13/2)组态带症称反转点变化主要原因的结论。过渡区核~(87)Zr的高自旋态研究在A≈80区，许多原子核的中子和质子数都处在28和50两个满壳层之间，对于这些核而言，任何一种核子数的改变都有可能导致核形状的显著变化。有研究结果表明，对于40≤Z≤45的核来讲，N=46是变形核向球形核变化的转折点。在40≤N≤50区，对Zr(Z=40)同位素系列中诸原子核能级结构伴随中子数改变而发生的变化的研究将会帮助我们了解这个形状变化的过程。我们所研究的~(87)Zr含有47个中子，就处于这个过渡区。实验是在北京中国原子能科学研究院HI-13串列加速器上进行的，利用入射能量为118MeV的~(32)S束通过~(58)Co(~(32)S,3pn)~(87)Zr熔合蒸发反应布居。~（87）Zr的高自旋态，实验用的靶为附有Ta衬的厚度1082μg／cm~2的~(59)Co箔。用7台HpGe探测器组成的探测阵列进行γ-γ符合测量。同时采用一个小平面光子探测器探测低能γ射线。本实验记录了约1.5 * 10。个两重以上的符合事件，建立了自旋直到37／2和43／2的能级纲图。研究的结果表明：~(87)Zr与相邻同中子奇A核的正宇称低激发能级之间存在着很强的相似性，而与相邻奇A核同位素相比，结构变化明显， 这可能表明在该核区对核形变的影响中子占主要地位，质子影响较小。激发能随中子变化的比值图呈阶梯状，认为R ≈ 1.5，R_x ≈ 2.0和R_x ≥ 2.2分别代表核形变的三个区域，即球型核、过渡区核和形变核。通过与相邻(Z,N + 1)偶偶核低激发态能级相比较的方法对各低激发能级组态的主要成分进行了估计，发现随自旋的增加，出现了各能级组态之间的混杂。