论爱因斯坦固体模型中声子的化学势

本文利用微正则系综求解了爱因斯坦固体的热力学性质,并说明了在微正则系综中无法独立定义爱因斯坦固体的声子数.在其他系综中,声子数量与温度相互独立,我们严格证明了此时声子的化学势为零.     

多粒子多空穴能态密度的谐振子模型计算

在严格考虑了泡利不相容原理的前提下,导出了任意单粒子哈密顿量下多粒子多空穴态的能态密度的一般性精确公式;并应用半经典的Thomas-Fermi近似,计算了三维线性谐振子下的能态密度;计算了g_1p至g_10p,g_1h至g_7h以及g_1p－1h至g_6p－6h能态密度;讨论了泡利不相容的影响,与微子模型中通用的等间隔模型的能态密度进行了比较.由计算结果看出,激子模型中通用的等间隔单粒子能级密度模式在由核子诱发的核反应中,是一很好的近似.     

Invar合金的电子化学势均衡判据

用二元团簇作为描述Invar合金的基本结构单元,运用"团簇共振"结构模型,建立起以某一已知二元团簇与连接原子按1:x比例连接,描述Invar合金的电子化学势均衡判据.给出了Invar合金成分的经验分子式,即Invar合金成分=[团簇]1(连接原子)x.运用此判据,解析了部分Invar合金成分.发现典型的Invar合金实验成分与经验分子式相符合,说明基于"团簇共振"模型的Invar合金的电子化学势判据很好地解释了Invar合金成分的形成规律.     

源于“团簇-共振”模型的理想金属玻璃电子化学势均衡

理想金属玻璃是指完全满足电子结构稳定性的金属玻璃. 在我们前期工作中提出的“团簇加连接原子"及理想金属玻璃的“团簇-共振"结构模型的 基础上, 本文指出理想金属玻璃应该满足电子化学势均衡判据, 可定量给出团簇与连接原子的比例, 最终确定了理想金属玻璃成分式[团簇](连接原子)_x. 运用此判据, 解析了Cu-Zr基和Co-B基块体金属玻璃, 实验确定的最佳形成能力成分满足电子化学势均衡.     

密度和温度相关的对称能

利用Hartree–Fock理论,基于扩展的Skyrme有效相互作用,在抛物线近似下,解析地给出了零温度时对称能的密度相关形式.同时讨论了对称能的温度相关性,发现对称能随着温度的升高而减小,在温度较低时,对称能强度系数与温度的关系能较好地符合抛物线规律.     

均匀微弱电场对带电费米子体系热容量和化学势的影响

从统计物理半经典(Thomas-Fermi)近似方法出发,研究均匀微弱电场中带电费米子体系的热力学性质,推导出了带电费米子体系的热容量和化学势随外电场场强的变化关系,给出了体系的热容量和化学势在高温和低温近似下的解析表达式,进而分析了均匀微弱电场对带电费米子体系热容量和化学势的影响.     

均匀微弱电场对带电费米子体系热容量和化学势的影响

从统计物理半经典(Thomas-Fermi)近似方法出发,研究均匀微弱电场中带电费米子体系的热力学性质,推导出了带电费米子体系的热容量和化学势随外电场场强的变化关系,给出了体系的热容量和化学势在高温和低温近似下的解析表达式,进而分析了均匀微弱电场对带电费米子体系热容量和化学势的影响.     

双光子非共振作用系统中纯度和密度算符间距的演化

研究了双光子非共振作用系统中纯度和密度算符间距的特性.讨论了相干光场与激发态二能级原子作用时失谐量对纯度和密度算符间距演化的影响.数值计算表明:失谐量对末态与初态的间距和原子与光场的缠结有调制作用.     

局域共振的光子、声子功能材料

介绍一种利用局域共振的原理制造人工光、声子结构材料的方法，此种方法不同于通常建立在布拉格散射基础上的光、声子晶体能带材料，但又表现出与之相同的物理特征，局域共振光、声子模型的优点是样品制作相对简单；不依赖于结构的周期性；可制备出亚波长的能隙结构，为微波及长波声波能带结构的制造提供了一种十分简便而有效的方法。     

三个热力学偏导数()、()和()等于系统化学势的又一证明方法

对三个热力学偏导数()、()和()等于系统化学势给出了又一种证明方法.     

Some Properties of πr Meson in Nuclear Matter with Finite Density

In the GCM we study some properties of π meson as the Goldstone bosons in a nuclear matter with finitedensity. Using the effective action in a nuclear matter, we calculate the decay constant and π mass as functions of thechemical potential. The relation between the chemical potential and the density of a nuclear matter is firstly given here.We find that fπ and mπ monotonously decrease as nuclear matter density increases. The result is consistent with theusual assumption that the chiral symmetry is gradually restored as the density of a nuclear matter increases.     

Large Number, Dark Matter, Dark Energy, and Superstructures in the Universe

Since there may exist dark matter particles ν and δ with mass - 10^-1 e V in the universe, the superstructures with a scale of 10^19 solar masses （large number A - 10^19） appeared during the era near and before the hydrogen recombination. Since there are superstructures in the universe, there may be no necessity for the existence of dark energy. For checking the superstructure in the universe by CMB anisotropy, we need to measure CMB angular power spectrum especially around ten degrees across the sky- in more details, While neutrino u is related to electroweak unification, the fourth stable elementary particle 6 may be related to strong-gravity unification, which suggests p ＋ p^- → n ＋ δ^- and that some new baryons appeared in the TeV region.     

Cosmological Relics of the High Energy Cold Dark Matter Particle in the Universe

We demonstrate that if the universe is dominated by the massive cold dark matter, then besides the generally believed thermal distribution of the dark matter relics, there may exist some very energetic nonthermal relics of the dark matter particles in the universe from some unknown sources, such as from decay of supermassive X particle released from topological defect collapse or annihilation. Very interesting, we point out that these high energy dark matter particles may be observable in the current and future cosmic ray experiments.     

核物质对称能的高密行为研究

同位旋物理的主要任务之一是通过放射性核束引起的核反应来探索介质中有效核子-核子相互作用的同位旋依赖性,尤其是同位旋相关的核物质状态方程, 即密度依赖的核物质对称能。由于对称能,尤其是其高密行为,对核物理学和天体物理学具有重要意义,密度依赖的对称能在过去10年一直是中能重离子物理研究领域的主要焦点之一。近年来,低密对称能的研究已经取得了重要进展, 而对称能的高密行为仍然很不确定。在理论方面,人们提出了许多对高密对称能敏感的观测量。 实验方面, 关于对称能高密行为研究的实验计划已经展开,世界各地正在建造的放射性核束装置为对称能的高密行为研究提供了新的机遇。基于IBUU输运模型综述了研究对称能高密行为的一些敏感观测量及其最新进展, 以及所面临的挑战与机遇。One of the major tasks of studying isospin physics via heavy ion collisions with neutron rich nuclei, is to explore the isospin dependence of in medium nuclear effective interactions and the equation of state of neutron rich nuclear matter, i.e., the density dependence of nuclear symmetry energy. Because of its great importance for understanding many phenomena in both nuclear physics and astrophysics, the study of the density dependence of nuclear symmetry energy has been the main focus of the intermediate energy heavy ion physics community during the last decade. Nowadays significant progress has been achieved in studying the low density behavior of nuclear symmetry energy, but the high density behavior of nuclear symmetry energy is still very uncertain. Theoretically, a number of observables have been proposed as sensitive probes to the high density behavior of nuclear symmetry energy. With new opportunities provided by the various radioactive beam facilities being constructed around the world, studies of the high density behavior of nuclear symmetry energy is expected to be one of the main forefront research areas in nuclear physics in the near future. In this report, based on the transport model IBUU we have reviewed the major progress achieved in studying the high density behavior of nuclear symmetry energy and discussed future challenges in this field.     

非对称核物质中同位旋对称势的动量和密度依赖性

在Brueckner-Hartree-Fock理论框架内, 研究了同位旋非对称核物质中质子和中子单粒子势的动量相关性及其随同位旋非对称度的变化, 在此基础上计算了同位旋对称势, 并讨论了三体核力的影响. 结果表明同位旋对称势对于同位旋非对称度的依赖性很弱, 但对于动量和密度均有较强的依赖性. 当密度固定时, 同位旋对称势随动量增加而减小. 尽管三体核力对于质子和中子单粒子势的动量相关性有较大影响, 但对同位旋对称势的影响很小. 还与目前重离子碰撞输运理论模型中所使用的各种参数化的唯象对称势进行了比较.     

Lindhard势与形变超晶格系统的共振现

假设超晶格“折沟道”对粒子的作用等效为形状相似的周期调制; 利用Lindhard 展开势, 并在小振幅近似下, 将面沟道粒子的运动行为化为了具有硬特性的弹簧振子。 利用多重尺度法分析了共振线附近的粒子运动行为, 讨论了系统的主共振、 子共振和超共振。 计算了超晶格“折沟道”临界斜率与系统参数之间的关系, 为研究超晶格光磁电效应提供了理论分析。It is assumed that a periodic modulation is equivalent to the deflected channel of the superlattice. In the small amplitude approximation the particle motion equation has been reduced to the Duffing equation with a hard-spring properties by using Lindhard expanded potential. The main resonance, the sub-harmonic resonance and the super-harmonic resonance have been analysed by the multi-scale technique. The critical parameter of the deflected channelling has been calculated, the results provided a theory analyse for the photo-magneto-electric effects of the superlattice.      

Chemical Potential Dependence of Vertices

Based on the rainbow-ladder approximation of the Dyson-Schwinger equations and the assumption of the analyticity of the fermion-boson vertex in the neighborhood of zero chemical potential (μ=0) and neglecting the μ-dependence of the dressed gluon propagator, we apply the method in [Phys. Rev. C 71 (2005) 015205] of studying the dressed quark propagator at finite chemical potential to prove that the general fermion-boson vertex at finite μ can also be obtained from the one at μ=0 by a simple shift of variables. Using this result we extend the results of [Phys. Lett. B 420 (1998) 267] to the situation of finite chemical potential and show that under the approximations we have taken, the Gell-Mann-Oakes-Renner relation also holds at finite chemical potential.     

能量密度泛函中不同对关联处理方式对原子核形变描述影响的探讨

在Skyrme能量密度泛函理论的框架下,研究了不同对关联处理近似,如Hartree-Fock-Bogoliubov(HFB)、Hartree-Fock-Bogoliubov Lipkin-Nogami (HFBLN)及在HFBLN基础上考虑粒子数投影,对于原子核势能曲面计算及基态结合能的影响。同时,也研究了不同对力,如体积对力、表面对力及混合对力对结果的影响。研究的对象为典型的双幻核16O,40Ca,100Sn和208Pb,它们的基态为球形;还有典型的形变核48Cr,也研究了相应的Cr和Fe同位素链的结合能,最后讨论了对超重核298Fl的势能面计算。研究发现,对关联基本不改变形变极小点,但是由于对关联能的引入,对结合能会带来几个MeV的修正能量,HFB、HFBLN及投影计算的修正能量逐渐递增。对关联可以改变位能面最小点附近曲线的软度,使得形变较小点变浅,而在HFBLN基础上考虑粒子数投影,又可以让形变极小点变得更加明显。对关联也降低了位垒高度。在相同对关联处理近似下,混合对力与体积对力计算的势能面结果相接近,表面对力带来了更多的对关联能,对关联的效果更加显著。     

核物质四阶对称能中的交换项相关物理

基于协变密度泛函（CDF）理论,核物质四阶对称能可以被分解为动能部分,同位旋单态势能部分以及同位旋三重态势能部分。交换项的引入明显改变了同位旋单态势能部分和同位旋三重态势能部分的密度行为,特别是来自同位旋标量介子-核子耦合道的交换项贡献提供了一个压制作用。作为一种有益的尝试,引入广义的对称能,可以更直观地统一描述核物质各阶对称能效应。The density dependence of nuclear fourth-order symmetry energy S₄ is studied within the covariant density functional (CDF) theory in terms of the kinetic energy, isospin-singlet, and isospin-triplet potential energy parts of the energy density functional. When the Fock diagram is introduced, it is found that both isospin-singlet and isospin-triplet components of the potential energy plays important roles in determining the fourth-order symmetry energy. Especially, an extra suppression, which comes from the Fock terms via isoscalar meson-nucleon coupling channels, is revealed in the isospin-triplet potential part of the fourth-order symmetry energy. As an useful attempt, the generalized symmetry energy is introduced to describe the various orders of nuclear symmetry energies in a visual and self-consistent way.     

理解暗能量和暗物质之间的相互作用

从热力学角度研究了暗能量和暗物质之间的相互作用. 假设相互作用是平衡态上的涨落并考虑此涨落导致的熵的修正, 导出了相互作用的物理表述, 把我们模型和观测结果作了比较.