丰中子核105Mo单中子带结构的识别

通过对重核²⁵²Cf自发裂变产生的瞬发γ谱的测量, 对丰中子核¹⁰⁵Mo的能级结构进行了研究. 除确认与扩展了基带转动带外, 新识别了3个转动带, 它们分别被指定为建立在Nilsson能级3/2⁺[411], 1/2⁺[411]和5/2⁺[413]轨道上的单中子激发带, 并对这些集体带的特性进行了讨论.     

奇A Tm同位素链及[411 1/2]带退耦参数性质的研究

用准粒子组态相关的宏观一微观推转模型计算了奇A核^157一173Tm同位素链的基态、低激发态形变以及这些核的[411 1/2]奇质子带的退耦参数,并与实验结果进行了比较,着重分析了γ形变对奇ATm同位素链的退耦参数的影响,进而指出¹⁵⁷Tm的退耦参数异常可能是由于带相互作用引起的,讨论了退耦参数对Nilsson参数和形变参数的敏感程度.     

一种改进的对力形式

通过引进一个关联因子提出了一种改进的对力形式,更合理地反映出短程关联的特点.解释了¹⁵⁷Tm的基态自旋为[411]1/2⁺这一实验事实.     

双奇核中π1/2－[541]⊙νi13/2带的系统学特征

通过束流能量为97MeV的¹⁵²Sm(¹⁹F,5n)¹⁶⁶Lu熔合蒸发反应,用在束γ(谱学方法研究了¹⁶⁶的高自旋态,建立了5条转动带,其中3条带是本实验中首次确定的.发现了π1/2^－[541]⊙ν5/2⁺[642]带的低自旋旋称反转现象,该带的反转点自旋值17.5h同A=170区奇奇核的π1/2^－[541]⊙νi_13/2带的反转点变化趋势非常相符.     

首次测定短寿命缺中子同位素153Er和157Yb的EC/β+衰变纲图

利用¹⁶O重离子束轰击¹⁴²Nd和¹⁴⁷Sm同位素靶分别生成¹⁵³Er和¹⁵⁷Yb.借助氦喷嘴带传输系统和X-γ、γ-γ符合测量方法分离鉴别核素并测量其衰变性质.首次建立了¹⁵³Er和¹⁵⁷Yb的EC/β⁺衰变纲图.从中指认出¹⁵³Ho的一个新三(准)粒子态和两个新单粒子态,指认出¹⁵⁷Tm的一个新的同质异能态和一条新转动带.低位能级系统分析表明:在Ho和Tm这两条奇A核的同位素链中基态形状的转变区都在中子数86和88之间.     

169Re的转动带结构研究

利用在束γ谱学方法,通过反应¹⁴⁴Sm(²⁸Si,1p3n)¹⁶⁹Re研究了¹⁶⁹Re的激发态能级结构.实验进行了X-γ符合、γ-γ符合、DCO系数和带内B(M1)/B(E2)比率测量.基于这些测量,建立了组态为π9/2^－[514]的强耦合带和组态为π1/2^－[541]的退耦合带.通过比较¹⁶⁹Re的转动带与邻近奇质子核已知转动带的结构和B(M1)/B(E2)比率,指定了¹⁶⁹Re转动带的组态.实验观测到π9/2^－[514]和π1/2^－[541]转动带的中子AB带交叉的转动频率分别为0.23和0.27MeV.着重讨论了¹⁶⁹Re转动带的中子AB带交叉频率、转动角动量顺排和旋称劈列等,并讨论了奇ARe核转动带结构的系统性     

187Pt的转动带性质研究

利用在束γ谱学技术和¹⁷³Yb(¹⁸O, 4n)熔合蒸发反应研究了¹⁸⁷Pt的高自旋态能级结构. 建立了包括3个转动带的¹⁸⁷Pt高自旋态能级纲图. 基于¹⁸⁷Pt周围核结构的系统学和比较带内B(M1)/B(E2)比率的实验值和理论值, 建议上述3个转动带的组态 分别为11/2⁺[615], 7/2^－[503]和1/2^－[521]. 对各转动带的带交叉频率、顺排增益、旋称劈裂等进行了讨论.     

171Lu 1/2－[541]轨道的形变驱动作用

通过熔合蒸发反应¹⁶⁰Gd(¹⁹F,6n2p)对¹⁷¹Lu的1/2^－[541]转动带进行了研究,观测到了此带的第一带交叉频率.与相邻偶偶核相比该频率值推迟了约40keV.推转壳模型对单准质子的顺排角动量和能量的计算结果表明πh_9/2[541]1/2^－轨道的形变驱动作用对这种推迟的贡献是不应被忽略的.     

157,159Tm基态附近性质的研究

利用可变转动惯量的三轴粒子-转子模型研究了^157,159Tm低激发正宇称态的性质,理论值和实验值比较好的符合表明¹⁵⁷Tm和¹⁵⁹Tm是三轴形变核,指出实验还给出了¹⁵⁷Tm另一条激发转动带.     

169Re的转动带结构组态相关性研究

研究了¹⁶⁹Re的高自旋态能级结构,建立了组态为π9/2^－[514]的强耦合带和组态为π1/2^－[541]的退耦合带,推转壳模型(Cranked shell model)计算结果表明组态相关的不同形变能够解释这些转动带的不同带交叉频率,在已知的奇ARe核中,¹⁶⁹Re的9/2^－[514]转动带在低自旋时具有最大的能量旋称劈裂,当一对i_13/2中子顺排后,旋称劈裂发生了反转,并且劈裂的幅度非常显著地减少了,另外,还观测到了一个三准粒子激发带,并指定了它的最可能组态为π9/2^－[514]⊙νAE。     

HBT参数对π源空间分布的敏感性研究(英文)

利用理想高斯源的两粒子关联函数，对单高斯源和双高斯源的两π介子HBT关联效应进行了研究，得出了相应的半径参数和A参数．结果表明，半径参数主要取决于高能重离子碰撞中多数π介子产生的中间区域；对产生π介子的边缘区域的空间分布形状不敏感．在边缘区域内产生的π介子主要影响A参数的变化．π介子源空间分布的非高斯形是导致λ参数减少的一个重要因素．The HBT radius parameters and the HBT λ-parameters of single Gaussian source and double Gaussian source are investigated by using two-pion correlation function in HBT intensity interferometry. It is indicated that the radius parameter is insensitive to the spatial shape of the edge zone of source and is mainly affected by the size of the central zone of pions emitted in high energy heavy-ion collisions. The pions produced at the edge of source influence the λ parameter. The non-Gaus...     

裂变位垒参数的推荐和裂变位垒参数库

通过分析和计算锕系核裂变截面和全套中子反应截面获取了一组锕系核的裂变位垒参数.Fm)在此基础上,广泛收集实验裂变位垒参数,通过比对和评价,推荐了本组的129个核素(109Cd—255的实验裂变位垒参数.此外,对收集的不同裂变位垒参数作了分析与评价,推荐了7组实验和1组模型计算的裂变位垒参数,并组建了中国评价核参数库裂变位垒参数子库(CENPL FBPL). The fission barrier parameters for actinide nuclei were obtained by analysis and calculations of fission cross-sections and complete neutron reaction cross sections. A lot of experimental fission barrier parameters from different authors were collected. A set of fission barrier parameters for 129 nuclei ranging from~(109)Cd~( ) to~(255)Fm were recommended after performing comparisons, evaluations and systematics extrapolations for these extracted fission barrier parameters in model calculations of fissi...     

Constraints on kinematic models from the latest observational data

Kinematical models are constrained by the latest observational data from geometry-distance measurements, which include 557 type Ia supernovae (SNIa) Union2 data and 15 observational Hubble data. Considering two parameterized deceleration parameter, the values of current deceleration parameter q₀$q_0$, jerk parameter j₀$j_0$ and transition redshift zT$z_T$, are obtained. Furthermore, we show the departures for two parameterized kinematical models from ΛCDM model according to the evolutions of jerk parameter j(z)$j(z)$. Also, it is shown that the constraint on jerk parameter j(z)$j(z)$ is weak by the current geometrical observed data.     

截断非傍轴双曲余弦-高斯光束的远场特性

基于瑞利-索末菲衍射积分公式,推导出截断非傍轴双曲余弦-高斯光束在自由空间传输的解析表示式,分析了一些特例,并引入非傍轴范畴的桶中功率概念,用以描述非傍轴光束的远场光束质量。结果表明:截断非傍轴双曲余弦-高斯光束的光强和桶中功率不仅与束腰宽度与波长之比、偏心参数及截断参数有关,而且桶中功率还与桶的尺寸有关。在一定的范围内,较大的束腰宽度与波长之比, 截断参数和较小的偏心参数使光束有更好的聚焦特性,表现出更好的光束质量。     

散射相函数的高阶光学参量研究

漫反射光谱技术被广泛应用于无创测量生物组织光学性质。当光源与探测器很近时,仅仅依靠吸收系数μ_a和约化散射系数μ′_s不能准确描述光源附近光的传播状态。而二阶光学参量γ的引入改善了近光源光的传播状态的描述。本文将生物组织的散射等效成特定球形颗粒的散射,基于Mie散射理论,计算了与散射相函数p(θ)有关的单粒子和多分散系粒子的二阶光学参量γ,研究了γ随尺度参数α和相对折射率m的变化规律,描述了γ与组织结构参量之间的联系,并阐述了γ对粒子特征的表征能力。研究表明,参量γ对尺度参数α小于2的微粒尺寸的改变是敏感的,并呈二次函数关系,其系数与相对折射率呈线性关系;对于相对折射率和尺度参数都不相同的两个粒子,他们的各向异性因子g相同时,二阶光学参量γ却不同,粒子越大,γ表征粒子特征的能力越强。这对于无创探究组织微观形态具有深远的意义。     

Effects of lattice dispersion and elastic anisotropy on the thermal properties of fcc metals

New parameters which separately take into account the effects of elastic anisotropy and phonon dispersion on the lattice specific heat in the case of fcc metals have been evaluated. A new graded mesh method which uses 162-direction approximation in (1/16) part of the Brillouin zone has been developed to evaluate the two new parameters.     

Viscous Fluid Cosmology in Bianchi Type-I Space-Time

The paper presents a spatially homogeneous and anisotropic Bianchi type-I cosmological model consisting of a dissipative fluid. The field equations are solved explicitly by using a law of variation for mean Hubble parameter, which is related to average scale factor and yields a constant value for deceleration parameter. We find that the constant value of deceleration parameter describes the different phases of the evolution of universe. A barotropic equation of state (p=γ ρ) together with a linear relation between shear viscosity and expansion scalar, is assumed. It is found that the viscosity plays a key role in the process of the isotropization of the universe. The presence of viscous term does not change the fundamental nature of initial singularity. The thermodynamical properties of the solutions are studied and the entropy distribution is also given explicitly.     

Prospect for Cosmological Parameter Estimation Using Future Hubble Parameter Measurements

We constrain cosmological parameters using only Hubble parameter data and quantify the impact of future Hubble parameter measurements on parameter estimation for the most typical dark energy models. We first constrain cosmological parameters using 52 current Hubble parameter data including the Hubble constant measurement from the Hubble Space Telescope. Then we simulate the baryon acoustic oscillation signals from WFIRST (Wide-Field Infrared Survey Telescope) covering the redshift range of z ∈[0.5,2] and the redshift drift data from E-ELT (European Extremely Large Telescope) in the redshift range of z ∈[2,5]. It is shown that solely using the current Hubble parameter data could give fairly good constraints on cosmological parameters. Compared to the current Hubble parameter data, with the WFIRST observation the H(z) constraints on dark energy would be improved slightly, while with the E-ELT observation the H(z) constraints on dark energy is enormously improved.     

A simple model to extract hyperfine interaction distributions from Mössbauer spectra

The general problem of finding a distribution in hyperfine interaction parameters from experimental Mössbauer spectra is outlined. Existing methods may lack flexibility to be easily applicable to simple problems. A line shape for hyperfine parameter distributions is given, which is based on linear segments in the probability function. This method is applied in the analysis of samples containing iron in a silicate glass.