回弯的简单公式

用吴-曾公式描述基带,用常转动惯量公式描述超带,且引入一个唯象的带间相互作用将两个带混合,即可得到对大多数原子核晕带较为理想的描述,还可重现转动惯量的回弯.对公式中的参数做进一步的分析后,可获得核的基态转动惯量与刚体转动惯量等信息.     

关于185Pt核多带结构的回弯机制

最近报道的¹⁸⁵Pt核多带结构的实验结果,又一次提出了其中五条带回弯现象究竟是由于h_9/2质子对转动排列所致,还是来自于i_13/2中子对转动排列结果的尖锐问题.基于阻塞效应的实验事实支持前者,而总罗斯量(转动坐标系中的总能量)而的理论计算则支持后者,本文在分析上述两种解释的前提条件的基础上,给出考虑了带交叉过程动力学效应的理论计算结果.说明了h_9/2质子对转动排列应是这五条带出现回弯的根源.     

双奇核136La的集体带结构

通过重离子核反应与在束γ谱的实验技术, 对A=130缺中子核区的双奇核¹³⁶La的高自旋态进行了研究, 所用核反应为¹³⁰Te(¹¹B,5n). 实验结果扩展了¹³⁶La的能级纲图, 包括3个集体转动带, 最高自旋态达20h. 对于\uppi h_{11/2}\otimes \upnu h_{11/2}$~带, 观测到了旋称反转与集体回弯现象. 通过系统学比较, 对旋称反转特性进行了讨论. 由推转壳模型的计算指出, 此集体回弯是由一对中子的角动量顺排引起的. 另外两个集体带为具有~$\gamma\approx -60^\circ$~的扁椭形变带, 其可能的组态为: $\uppi h_{11/2}\otimes \upnu g_{7/2}h_{11/2}^2$~与~$\uppi g_{7/2}\otimes\upnu g_{7/2}^2 d_{5/2} h_{11/2}^2$.     

80Rb的旋称劈裂反转及负宇称带的回弯

通过熔合蒸发反应⁶⁵Cu+¹⁹F,⁶⁶Zn+¹⁸O及⁶⁸Zn+¹⁶O,在3种入射束流的能量分别为75MeV,76MeV及80MeV研究了⁸⁰Rb高自旋态的能级结构.增加了20多条新的γ跃迁,在已知负宇称转晕带上建立了两条新的边带.将原有的第二条负宇称带的自旋态从12^－推高到了22^－,并首次观察到这个带的回弯,它的回弯频率为0.49MeV;负宇称转晕带在15^－时出现了旋称反转,第二负宇称带存在明显的旋称劈裂,但没有观察到旋称反转,这两条负宇称带的结构均与其同中子数核⁸²Y非常相似.     

含三体势的IBM1的O(6)极限对偶偶120～130Xe和124～130Ba核的Yrast带回弯研究

应用含三体势的ＩＢＭ１的Ｏ（６）极限［Ｏ（６）＋Ｖ３］对过渡区偶偶核１２３～１３０Ｘｅ、１２４～１３０Ｂａ的Ｙｒａｓｔ带能谱和回弯现象进行了分析研究．结果表明:Ｏ（６）＋Ｖ３能较好地描述回弯的主要特征.The Yrast band energy spectra of even even nuclei 120～130 Xe and 124～130 Ba are calculated by using the O (6) limit of IBM1 containing three body potential. It shows that the backbending characteristics in the Yrast bands can be described fairly by O (6)+ V 3 .     

85Zr核的高自旋态研究

利用102MeV的28Si束流,通过60Ni(28Si,2pn)熔合蒸发反应布居了85Zr核的高自旋态,测量了γ-γ符合及DCO比值,建立了一个有43条能级,75条γ跃迁的能级纲图,新增加了36条γ跃迁,25条能级.将能级自旋推高到(49/2+),首次观察到了转晕带的第二回弯.并确认了一条建立在17/2-负宇称带上的磁转动带.     

q形变三参数吴曾公式

结合微扰论的结果详细分析了描述偶偶核基带能谱三参数吴曾公式的q形变形式. 运用阻危非线性最小二乘法对大部分稀土区和锕系区的偶偶核基带能谱进行了拟合. 计算结果表明,q形变三参数吴曾公式比原来从微扰论导出的三参数吴曾公式更为精确,并能较好地描述回弯现象.     

125Ba高自旋态的测量

通过¹⁰⁹Ag(¹⁹F,3n)核反应布局了¹²⁵Ba核的激发态.使用带BGO康普顿抑制的高纯锗探测器阵列和常规在束γ实验技术,测量了它的高自旋态.建立在h_11/2中子支壳上的负宇称带和建立在g_7/2中子支壳上的正宇称带分别被延伸到了35/2^－和23/2⁺态.负宇称带显示出明显的正负Signature劈裂,而正宇称带则几乎没有这种劈裂.负宇称正负Signature带均出现反弯,其反弯处转动频率与¹²⁴Ba晕带反弯频率相近.正宇称带出开始出现反弯迹象.     

^95Zr核的高自旋态研究

利用102MeV的^28Si束流，通过^60Ni(^28Si，2pn)熔合蒸发反应布居了^85Zr核的高自旋态，测量了γ-γ符合及DCO比值，建立了一个有43条能级，75条γ跃迁的能级纲图，新增加了36条γ跃迁，25条能级。将能级自旋推高到（49/2^ ），首次观察到了转边带的第二回弯。并确认了一条建立在17/2^-负字称带上的磁转动带。     

134Ba核的高激发态能级结构研究

在中国原子能科学研究院H-13串列加速器上, 通过重离子核反应¹³⁰Te(⁹Be,5n)与在束γ谱的实验技术, 对A=130缺中子核区的¹³⁴Ba核的高自旋态进行了研究, 建立了¹³⁴Ba核的新的能级纲图, 最高自旋态扩展到20h. 除验证了以前报道的大部分能级与跃迁外, 将基带的能级扩展到10⁺, 同时发现了基于10⁺同质异能态以上的众多的能级与跃迁. 对实验结果的系统学分析表明, 10⁺同质异能态为yrast陷阱, 起源于两中子组态, 可能具有γ≈－120°的长椭形状, 在其以上的能级表现出很强的单粒子性，具有复杂的结构. 基带中观测到明显的集体回弯现象, 推转壳模型的计算表明, 此集体回弯是由一对中子的顺排所致, TRS计算表明, 随着转动频率的增加, 核的形状发生明显的变化, 基带中在中子顺排后核具有γ≈－60°的扁椭形状.     

192Tl高自旋态能级结构研究

通过熔合蒸发反应181Ta（16O,5n）192Tl,在入射束流为97 MeV能量下,布居192Tl的高自旋态,更新了192Tl的能级纲图。共增加8条新能级,尝试性地指定了能级自旋,将负宇称晕带的能级推高到23-?。讨论了192Tl与相邻同位素奇奇核194,196,198Tl负宇称晕带的旋称劈裂与反转现象,发现随着中子数增加,196,198Tl在高自旋处出现了旋称反转,其原因可能是由于中子质子相互作用与科里奥利力相互竞争所致。High spin states of 192Tl were populated by the 181Ta(16O, 5n)192Tl heavy ion fusion evaporation reaction at 97 MeV beam energy. A new level scheme with 8 new levels was constructed and the level spins were tentatively assigned. The negative yrast band was extended up to 23-?. Systematics of signature of inversion were also discussed for the negative yrast band of odd-odd Tl istopes. Signature inversion has been found in 196,198Tl with neutron number increasing in these four Tl isotopes, and it is explained by the competition between the strength of n-p interaction and Coriolis force.     

Backbendings of superdeformed bands in ~(36,40)Ar

Experimentally observed superdeformed(SD) rotational bands in ~(36)Ar and ~(40)Ar are studied by the cranked shell model(CSM) with the pairing correlations treated by a particle-number-conserving(PNC) method.This is the first time that PNC-CSM calculations have been performed on the light nuclear mass region around A=40.The experimental kinematic moments of inertia J~((1))versus rotational frequency are reproduced well. The backbending of the SD band at frequency around ω =1.5 Me V in ~(36)Ar is attributed to the sharp rise of the simultaneous alignments of the neutron and proton 1 d_(5/2)[202]5/2 pairs and 1 f_(7/2)[321]3/2 pairs, which is a consequence of the band crossing between the 1 d_(5/2)[202]5/2 and 1 f_(7/2)[321]3/2 configuration states. The gentle upbending at low frequency of the SD band in ~(40)Ar is mainly affected by the alignments of the neutron 1 f_(7/2)[321]3/2 pairs and proton 1 d_(5/2)[202]5/2 pairs.The PNC-CSM calculations show that besides the diagonal parts, the off-diagonal parts of the alignments play an important role in the rotational behavior of the SD bands.     

Proton Orbital [541]1/2 and Backbending in 178W

The microscopic mechanism of nine experimentally observed bands in ¹⁷⁸W is investigated using the particle-number conserving method of the cranked shell model with monopole and quadrupole paring interactions. The experimental results, including the moments of inertia and angular momentum alignments of nine bands in ¹⁷⁸W, are reproduced well by the particle-number conserving calculations, in which no free parameter is involved. Calculations demonstrate that occurrence of sharp backbending comes mainly from the contribution of high-j intruder orbitals νi13/2 or πh11/2 and their interference effect with orbitals near the Fermi surface. The ω variation of the occupation probability of each cranked orbital and the contribution to moment of inertia from each cranked orbital are analyzed.     

Proton Orbital [541]1/2 and Backbending in 178W

The microscopic mechanism of nine experimentally observed bands in ^178W is investigated using the particle-number conserving method of the cranked shell model with monopole and quadrupole paring interactions. The experimental results, including the moments of inertia and angular momentum alignments of nine bands in ^178W, are reproduced well by the particle-number conserving calculations, in which no free parameter is involved. Calculations demonstrate that occurrence of sharp backbending comes mainly from the contribution of high-j intruder orbitals vi13/2 or πh11/2 and their interference effect with orbitals near the Fermi surface. Theω variation of the occupation probability of each cranked orbital and the contribution to moment of inertia from each cranked orbital are analyzed.     

Guided-Wave Two-Dimensional Acousto-Optic Scanner Using Proton-Exchanged Lithium Niobate Waveguide

Two-dimensional scanning of a 0.6328 mum guided-light beam has been realized using noncolinear acousto-optic (AO) coplanar Bragg diffraction together with colinear AO guided-mode to substrate radiation-mode conversion in a Z-cut Xpropagation LiNbO3 proton-exchanged (PE) waveguide. The two surface acoustic (SAW) waves utilized are at the center frequencies of 500 and 200 MHz, propagating in the Y and X axes, respectively. Two-dimensional scanning of approximately 720 resolvable light beam spots, namely, 18 40 (horizontal vertical) scanning, has been demonstrated using a light beam of 1.0 mm aperture. The total number of resolvable beam spots can be greatly increased from 720 by simply utilizing SAW transducers of larger bandwidth and a light beam of greater aperture. It should also be possible to significantly increase the diffraction efficiency from 3 % by optimizing the parameters of the PE waveguide and the SAWs.     

Femtosecond Transform-Limited Pulse Generation by Compensating for the Linear Chirp of SPM Spectra in Dispersion Shifted Fibers

A simple technique of pulse compression, based on the linear chirp compensation of self-phase modulation (SPM) spectra in dispersion shifted fibers, is demonstrated. The optimization procedure is carried out, for a short span of a single-mode fiber, using a parabolic law, which describes the behavior of the squared output pulse width versus the pump peak power in the case of Gaussian pulses. The experimental results give a minimum pulse duration of 233 fs, which is in good agreement with the model. Shorter and coherent pulses, down to 90 fs, have been obtained by inserting an interference filter at the optical output.     

Effect ofγ-radiation on the spectral luminescence characteristics of impure cadmium tungstate crystals

Results of a study of the effect of γ-radiation on the spectral luminescence properties of cadmium tungstate crystals doped with silver, bismuth, and molybdenum cations are presented. Spectral characteristics of the nondnnnoped crystals are briefly described. Absorption and photo and X-ray luminescence spectra of the crystals taken before and after exposure to γ-radiation (5.5·10⁴ Gy) are compared. It is found that the spectral characteristics of the crystals doped with silver, bismuth, and molybdenum cations do not change markedly after the exposure. The relation between the type of impurity-induced defects, individual characteristics of the impurity cations, and the character of the effect of γ-radiation on the spectral luminescence properties of impure crystals is analyzed (preliminarily). Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 64, No. 1, pp. 55–60, January–February, 1997.