转动对电磁跃迁的影响——带交叉以后的区域

利用推广的粒子-转子模型研究了¹⁵⁹Tm负宇称Yrast态在带交叉以后区域的B(M1)值以及动力学电四极矩Q⁽¹⁾和Q⁽²⁾,并同实验进行了比较,得到了较好的符合,指出二级柯里奥利作用对分析实验数据的重要性.     

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.     

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.     

高自旋态下160Lu能级自旋的确定

通过¹⁴⁴Sm(¹⁹F,3n)反应对¹⁶⁰Lu高自旋态进行了研究.首次建立了¹⁶⁰Lu高自旋态能级纲图.依据相加性法则对¹⁶⁰Lu各能级的自旋及宇称进行了讨论.     

转动对电磁跃迁的影响

利用推广的粒子-转子模型研究了¹⁵⁹Tm负宇称Yrast态的能谱的Signature分离,B(M1)值以及动力学电四极矩Q^(1)和Q⁽²⁾,并同实验进行了比较,得到了较好的符合.着重分析了二级柯里奥利作用H_c对B(M1)值的Signature依赖性的影响,指出粒子-转子高级耦合项部分地等效于γ形变.     

锕系核集体运动的负宇称态

从锕系区40多个核的正负宇称态的实验数据,如激发能、J^π、电偶极跃迁等,得到一系列与核结构有关的物理量,如宇称劈裂能级差δE_I,正负宇称带的第一和第二类转动惯量J⁽¹⁾和J⁽²⁾及第一负宇称态的电偶极跃迁强度比等,以及它们与角动量I或转动角频率ω的动力学和核子数A的系统行为,从而为研究锕系核负宇称态的产生机制及动力学特点提供了信息.     

具有双Y-型结构的Θ+的研究

采用由单胶子交换产生的库仑势加上流管模型给出的双Y-型禁闭势之和的相互作用势,分别计算了正、负宇称态的Θ⁺的质量, 给出负宇称态Θ⁺的质量为1.935GeV, 正宇称态Θ⁺的质量为2.082GeV. 其中较低的负宇称态仍比实验给出的Θ⁺(1540)的共振峰高出近400MeV.     

A～100区Tc同位素能级结构的研究

用投影壳模型对¹⁰¹Tc的受激正/负宇称转晕态结构进行了探讨, 为了从定量结果中抽取出物理内容也作出了正宇称转晕带的能带图. 此外, 各自起源于3/2^－[301], 5/2^－[303]和1/2⁺[431]尼尔逊态的3个带也在这个模型框架下进行了分析. 到目前为止, 在Z～42—44区关于N=52—54的中间核性质知之甚少, 为了解这些"过渡核", 以⁹⁵Tc为例, 对其能级结构也进行了研究.     

162Lu的高自旋态及A=160区双奇核晕态能级的符号因子反转

利用¹⁴⁷Sm(¹⁹F,4nγ)¹⁶²Lu反应研究了¹⁶²Lu的高自旋态. 由7个带BGO康普顿抑制的高纯锗探测器和一个小平面探测器进行了在束γ测量,首次建立了双奇核¹⁶²Lu转晕带的能级纲图. 发现在低转动频率下,¹⁶²Lu的转晕带能级发生符号因子反转. 对质量数A=160核区双音核的转晕带重新进行了分析和考察,讨论了转晕带能级符号因子反转的系统性.     

135La高自旋态的实验研究

利用在束γ谱实验技术,通过¹²⁸Te(¹⁰B,3n)¹³⁵La反应研究了¹³⁵La的高自旋态.基于γγ符合关系、γ射线的相对强度和各向异性度的测量结果,建立了¹³⁵La的能级纲图.在hω≈0.40MeV附近,观测到基于πh_11/2质子轨道上的负宇称带的带交叉.比较N=78同中子素链能级结构的系统性,认为该带交叉是由一对h_11/2准质子发生转动顺排造成的.在高自旋态处,观测到具有很强M1跃迁、Signature劈裂很小的ΔI=1负宇称带,根据系统性认为该带是建立在πh_11/2(νh_11/2)²组态上的γ≈–60°的扁椭球形变带.     

Instability of the quasi-particle vacuum and band-crossing in high-spin rotational states

It is shown that the energy of the quasi-particle excitation in a rotational system may become negative when the angular frequency ω reaches a certain value. As a result, the energy of the excited state may be lower than the energy of the quasi-particle vacuum. It is suggested that this may serve as a natural explanation of the recently observed band-crossing phenomena where the levels of the “excited-band” become lower then the levels of the “ground-band” after a certain value of angular momentum. Preliminary calculation agrees well with the experimental result obtained in Juelich for ¹⁵⁶Dy.     

The reversibility of the Goos–Hänchen shift near the band-crossing structure of one-dimensional photonic crystals containing left-handed metamaterials

We perform a theoretical investigation on the Goos–Hänchen (GH) shift in one-dimensional photonic crystals (1DPCs) containing left-handed metamaterials (LHMs). We find an unusual effect of the GH shift near the photonic band-crossing structure, which is located at the condition, ?k _z ^(A) d _A =k _z ^(B) d _B =m π (m=1,2,3,…), under the inclined incident angle, here A denotes the LHM layer and B denotes the dielectric layer. Above the frequency of the band-crossing point (BCP), the GH shift changes from negative to positive as the incident angle increases, while the GH shift changes reversely below the BCP frequency. This effect is explained in terms of the phase property of the band-crossing structure.     

Cranking model interpretation of weakly coupled bands in Hg isotopes

The positive-parity yrast states of the transitional ^189–198Hg isotopes are interpreted within the Bengtsson and Frauendorf version of the cranking model. The very sharp backbendings can be explained by small interaction matrix elements between the ground and s-bands. The experimentally observed large aligned angular momenta and the low band-crossing frequencies are well reproduced in the calculations.     

Rotation aligned bands and configuration dependent interaction in189Hg

High spin states in¹⁸⁹Hg have been studied using the¹⁸¹Ta(¹⁴N, 6n) reaction. The various one- and three-quasiparticle rotational bands were interpreted within the cranked shell model. The band-crossing frequencies are found to depend on the number of spectator particles. The effect can be accounted for by a residual two-body interaction of appr. ?0.11 MeV.     

First observation of yrast band in odd-odd 162Lu

High spin states of the odd-odd ¹⁶²Lu nucleus have been studied via ¹⁴⁷Sm(¹⁹F,4nγ)¹⁶²Lu reaction at 95 MeV beam energy. Level scheme for yrast band based on π[h_11/2]υ[i_13/2] quasiparticle configuration was established up to I^π=(23^?) for the first time. This band shows the signature inversion in energy before backbending generally appeared in this mass region. It is stressed that the signature splitting in ¹⁶²Lu is larger than that in the ¹⁶⁰Tm nucleus.     

稀土元素Lu，Sc掺杂GaN光电特性的第一性原理研究

基于密度泛函理论，采用广义梯度近似（GGA+U）平面波超软赝势方法，计算了本征GaN和稀土元素Lu、Sc掺杂GaN体系的电子结构和光学性质.结果表明：计算得到本征GaN的禁带宽度为3.37 eV，与实验值（3.39 eV）接近. Lu掺杂后GaN体系带隙变窄，而Sc掺杂后诱导了深能级杂质，带隙变宽，但仍为直接带隙半导体.掺杂后体系均发生畸变，晶格常数和体积增大，且在费米能级附近产生杂质带. Lu、Sc掺杂GaN体系的静态介电常数较本征GaN（4.50）均有所增大.Lu、Sc掺杂后体系介电常数虚部整体左移，光吸收边往低能方向移动，发生了红移现象.计算结果对稀土元素Lu、Sc掺杂GaN高压光电材料的开发和研究提供了理论依据.     

First observation of yrast band in odd-odd162Lu

High spin states of the odd-odd¹⁶²Lu nucleus have been studied via¹⁴⁷Sm(¹⁹F,4nγ)¹⁶²Lu reaction at 95 MeV beam energy. Level scheme for yrast band based onπ[h_11/2 v[i_13/2] quasiparticle configuration was established up to I ^π = (23^?) for the first time. This band shows the signature inversion in energy before backbending generally appeared in this mass region. It is stressed that the signature splitting in¹⁶²Lu is larger than that in the¹⁶⁰Tm nucleus.     

Lu2Si2O7∶Ce纳米晶的溶胶-凝胶法合成和闪烁性能

采用溶胶-凝胶法制备了Lu2Si2O7∶Ce纳米晶,利用X射线衍射(XRD)、扫描电镜(SEM)、荧光光谱仪、X射线激发发射谱仪对制备的Lu2Si2O7∶Ce纳米晶的晶相结构、微观形貌和光学性能进行了表征。结果表明,溶胶-凝胶法制备的Lu2Si2O7∶Ce前驱体在煅烧温度为1000℃时开始晶化,晶粒尺寸随着煅烧温度的升高而变大,1200℃煅烧2 h后的晶体颗粒均匀,分散性最优,平均晶粒尺寸约为28.9 nm,呈近球形;Lu2Si2O7∶Ce纳米晶的紫外吸收谱存在峰位分别为304 nm和350 nm两个吸收峰,源自于Ce^3+离子的4f→5d跃迁;光致发射谱和X射线激发发射谱都表现为典型的非对称双峰结构,归属于Ce^3+离子的5d^1→2F5/2和5d^1→2F7/2跃迁,Ce^3+离子的最佳掺杂浓度约为1%;荧光衰减时间约为37.2 ns,可满足高时间分辨X射线探测需要。     

Contrasting high-spin yrast bands in 172Os and 174Os and an unexpected low-frequency anomaly in 172Os

The yrast bands of the neutron deficient isotopes ¹⁷²Os and ¹⁷⁴Os have been identified to spins of about 24. The yrast band in ¹⁷⁴Os shows no bandcrossing anomalies, confirming the shell effect observed in other N = 98 nuclei. In contrast, a strong backbend observed at a frequency of about 0.26 MeV in ¹⁷²Os is attributed to the s-band crossing. A weaker band-crossing is also observed at a lower frequency, about 0.24 MeV, in ¹⁷²Os. This unexpected anomaly may be due to either a deformation effect, or to a change in the s-band structure.     

High spin states in the ground and β-bands of 156Dy and the band-crossing interpretation of back bending

High spin states have been identified in ¹⁵⁶Dy using (HI, xn) reactions and γ-γ coincidence techniques. The ground state band does not show any “phase change” or “back bending” behaviour up to spin 18⁺. However a second sequence, based on the β-vibrational band, does show back bending at spin 12⁺. The two sequences intersect just below spin 16⁺ with the 16⁺, 18⁺ and 20⁺ members of the β-band sequence becoming yrast levels. Branching ratios have been obtained for transitions above and below the bend at spin 12⁺. The data are discussed in terms of a simple band-crossing model of back bending.