The Heisenberg Model after an Interaction Quench

In accordance with the recent experimental progress of the controllable spin-spin interactions, the Heisenberg model after an interaction quench is discussed. The Hamiltonian of the system out of equilibrium is introduced and treated by the flow equation method. As a result, the spectrum and zero-point spin deviation are obtained with the help of time-evolved operators. Additionally, other methods are applied to verify the results in mathematics. It is found that the observables show an oscillating behavior. The feasible experimental scheme of the concerned scenario is also mentioned.     

An Exotic Type of Fulde-Ferrel-Larkin-Ovchinnikov States in Spin-Orbit Coupled Condensates

We find for the first time that a model Hamiltonian or s-wave superconductors in tne presence or spm-orbit interactions and a Zeeman field is exactly solvable. Most intriguingly, based on the exact solutions, a novel type of Fulde Ferrel-Larkin-Ovchinnikov ground state is rigorously revealed, in which the center-of-mass momentum of the fermion pair is proportional to the Zeeman field. We also generalize our exact analysis to the spin-orbit- coupled Bose-Einstein condensate.     

Interactions between Solitons and Cnoidal Periodic Waves of the Gardner Equation

The Gardner equation is one of the most important prototypic models in nonlinear physics. Many scholars pay much attention to the Gardner equation and various nonlinear excitations of the Gardner equation have been found by many methods. However, it is very difficult to find interaction solutions among different types of nonlinear excitations. In this work, with the help of the Riccati equation, the Gardner equation is solved by the consistent Riccati expansion. Furthermore, we obtain the soliton-cnoidal wave interaction solutions of the Gardner equation.     

Interplay between External Strain and Oxygen Vacancies on Raman Spectra of SnO2

Comprehensive first-principle calculations on strained SnO2 crystal structure indicate that the formation energy of different types of oxygen vacancies depends on the external strain. Many novel Raman modes can be observed, their intensities and positions are strongly dependent on applied stain, which can be ascribed to crystal symmetry destruction by oxygen vacancies. Applied strain can compress/stretch distances between Sn and O atoms; therefore, Sn-O band vibration frequencies can be adjusted accordingly. Our calculated results disclose that the Raman spectra of SnO2 crystal structure with different types of oxygen vacancies are obviously different, which can be used to identify the oxygen vacancy types in strained Sn02 crystal structures.     

二氧化钒强关联固体的三相点

<正>在强关联材料中,电子—电子,电子—晶格的相互作用可导致各种电子相、磁相以及结构相之间的竞争。研究在这些竞争相之间的相变,往往可以揭示出用其他方法难以获得的有关基础量子态的信息。最近,来自美国华盛顿大学的Park等在Nature周刊上撰文,报道了他们使用微机械设备和纳米单晶束所完成的实验:在二氧化钒     

含有四个夸克或更多夸克的奇特粒子

<正>在粒子物理的所谓"标准模型"中发生强相互作用的基本粒子是带有分数电荷的夸克,这些夸克被电中性的类似光子的"胶子"捆绑在一起形成强子(包括重子和介子)。目前标准模型中包含6种不同"味道"的夸克:上夸克(u)、下夸克(d)、奇异夸克(s)、粲夸克(c)、底夸克(b)和顶夸克(t);它们各自的反粒子(反夸克)被标志为、d、、、、。每一种味道的夸克又带有强作用的3种不同的"色荷"之一的"色荷"。之所以称之为"色荷"是因为强相互作用将这些带色荷的夸克束缚在一起形成强子的法则很容易让我们类比到对颜色的感知。     

强磁场中相互作用费米气体的相对论稳定性

由单粒子的弱相互作用能谱及泊松公式,导出了强磁场中相互作用费米气体的相对论热力学势函数,求解了系统力学稳定性的判别式,分析了相互作用、磁场及相对论效应对系统稳定性的影响机理。结果表明,强磁场中弱相互作用费米气体的力学稳定性会受到弱相互作用的影响,强磁场对这种影响具有调节作用,而相对论效应对相互作用的影响基本没有调节作用。     

带有三体相互作用的XXZ自旋链模型的隐形传态

本文对基于海森堡XXZ自旋链模型的隐形传态的平均保真度进行了详细计算和分析.通过比较不带三体相互作用、仅带一种三体相互作用和同时带两种三体相互作用的各种海森堡铁磁质和反铁磁质XXZ模型在外磁场正向和反向时的保真度与外磁场和温度的关系,找到了一些理想模型,用这些模型进行隐形传态时需要的外界磁场相对较弱、温度相对较高,这个结论为实验上用海森堡XXZ模型进行隐形传态提供了很好的理论依据.     

SiS低激发态势能曲线和光谱性质的全电子组态相互作用方法研究

基于全电子的相关一致极化4-ζ(aug-cc-pwCVQZ-DK)基组,采用高精度的多参考组态相互作用方法计算了SiS自由基与最低的解离极限Si(3Pg)+S(3Pg)对应的18个Λ-S电子态的势能曲线.计算中考虑了标量相对论效应以及Si(2s22p6)和S(2s22p6)内壳层电子产生的关联效应.基于计算的势能曲线,拟合出了束缚态的光谱参数,包括平衡核间距Re,绝热激发能Te,振动常数ωe和ωeχe,平衡转动常数Be;并分析了束缚态在不同键长位置处的电子组态.计算了18个Λ-S态的电偶极矩函数,阐明了电子态的组态变化对电偶极矩的影响.给出了包含b3Π和A1Π态的自旋-轨道矩阵元随核间距变化的曲线,分析了邻近的电子激发态对b3Π和A1Π态的扰动.计算了A1Π—X1Σ+和E1Σ+—X1Σ+跃迁的跃迁偶极矩和Franck-Condon因子,讨论了A1Π和E1Σ+的最低五个振动能级的辐射寿命.     

评论:“边界振动的微腔中的二能级原子”

<正>在曲照军等的文章中[1]作者声称他们能够解决腔场影响原子问题.在此我们显示出既然他们用于得到相互作用表象的哈密顿的变换不完备所以他们没有解决该问题.我们知道此相互作用的哈密顿量可表示为(h=1)H=ωa■a+ωmb■b+ω0/2σz+g1(a■σ_+σ+a)+g2a■a(b■+b),(1)这里a和a■是单模量子化场的产生与湮灭算符,而b和b■为量子谐振子的产生与湮灭算符,g1是单模辐射场与原子的乡耦合系数,g2是单模辐射场与振动边界的耦合常数.曲照军等人把哈密顿量(1)分解成自由和相互作用两个哈密顿量H=H0+HI.这里