含时的线性驱动简并参量放大系统的量子起伏

导出在P表象中含时的线性驱动简并参量放大Fokker-Planck方程，并求其解.在阈值以下或阈值附近，含时驱动Fokker-Planck方程的解与线性理论或阈值附近的微扰理论预言的基本相符.在阈值以上，含时驱动Fokker-Planck方程解的短期行为也与线性近似解相近，但当τ增大后的长期行为完全区别于线性理论的结果. 关键词： 含时的线性驱动简并参量放大 Fokker-Planck方程 量子起伏     

新纠缠态表象的构建及其性质

运用有序算符内积分(IWOP)技术,构建了(x)2—p1和.(x)1—P2的共同本征态｜η〉,并分析了该新纠缠表象的Schmidt分解形式.另外,我们还得到纠缠态｜η>的共轭态｜ξ〉,同时计算了它们的内积.最后我们给出了新双模压缩算符S2=μ∫d2η/π｜μη〉〈η｜的显式,并分析了其压缩特性.     

双参数变形振子光场与物质相互作用的非线性理论

本文建立了双参数变形振子光场与物质相互作用的非线性理论,得到了相互作用表象中Schrdinger方程的形式解,并用微扰法求出了一级近似的发射概率和吸收概率,同时求解了共振条件的拉比问题,在q→1、s→1时,该理论恢复为普通线性理论。     

量子耗散微扰方法的适用性

将微扰量子耗散理论得出的两态线性吸收光谱与严格结果相比较. 所考虑的近似理论为两套完备两阶量子耗散方程,其一为标准的编时微扰方法,另一为所谓的完备二阶驱动耗散耦合方程. 对于两态线性吸收光谱,可以得到解析解,将结果与严格公式比较,来评估这两种方法的适用性和应用范围.     

在|η〉表象中求激子能级的非微扰严格解

我们在一个新的完备正交连续表象即｜η〉表象中严格求解了处于一般能带面的激子能级问题,而以往的标准作法是用ｋ·ｐ 微扰论计算到ｋ 的二级微扰的贡献．我们的结果表明了ｋ·ｐ 微扰论中高级微扰的贡献实际为零．     

q振子光场模型的光与物质相互作用的非线性理论

建立了一个以q振子为光场模型的光与物质相互作用的非线性理论,求得了薛定谔方程的形式解,并用微扰法求出一级近似的发射概率和吸收概率,同时求解了共振条件的拉比问题。在q→1时,恢复为普通线性理论。 关键词：     

无反射势阱的非齐次Schrdinger方程的精确解

无反射势阱描述一种双原子分子的吸引势。将Rayleigh Schr dinger展开法应用到微扰无反射势阱 ,得到一组非齐次Schr dinger方程。利用最近报道的微扰方法 ,导出这些方程的积分形式的精确解。以静电场与基态系统的相互作用为例 ,通过精确解的有界及其不能在Hilbert空间展开为有限项的性质 ,论证了该微扰系统束缚态的存在性及通常量子力学发散困难的起因。     

磁绝缘传输线振荡器中辐射场的非线性行为

导出了磁绝缘传输线振荡器 (MILO)中辐射场的非线性演化方程 ,并讨论了在临界值点附近可能出现非线性不稳定解的条件。结论是 :(1)非线性增长速率与线性增长速率的比值g <1.2 ,且远离 g γ =1(γ为非线性相位增长率与线性相位增长率的比值 )点时 ,出现非稳定解的失谐量临界值很小 ,而线性增长速率临界值临界值很大 ,容易出现非稳定解 ;(2 )当 g≥ 1.2时 ,任意小的失谐量都可以使场出现非稳定解 ;(3)线性增长速率越大 ,越不容易出现非稳定解     

无反射势阱的非齐次Schr(o)dinger方程的精确解

无反射势阱描述一种双原子分子的吸引势。将Ｒａｙｌｅｉｇｈ－Ｓｃｈｒｏｄｉｎｇｅｒ展开法应用到微扰无反射势阱,得以一组非齐次Ｓｃｈｒｏｄｉｎｇｅｒ方程。利用最近报道的微扰方法,导出这些方程的积分形式的精确解。以静电场与基态系统的相互作用为例,通过精确解的有界及其不能在Ｈｉｌｂｅｒｔ空间展开为有限项的性质,论证了该微扰系统束缚态的存在性及通常量子力学发散困难的起因。     

磁绝缘传输线振荡器中辐射场的非线性行为

 导出了磁绝缘传输线振荡器(MILO)中辐射场的非线性演化方程，并讨论了在临界值点附近可能出现非线性不稳定解的条件。结论是：(1)非线性增长速率与线性增长速率的比值g<1.2，且远离g+γ=1(γ为非线性相位增长率与线性相位增长率的比值)点时，出现非稳定解的失谐量临界值很小，而线性增长速率临界值临界值很大，容易出现非稳定解；(2)当g≥1.2时，任意小的失谐量都可以使场出现非稳定解；(3)线性增长速率越大，越不容易出现非稳定解。     

广义非简谐振子的多尺度微扰理论

应用多尺度微扰理论到广义非简谐振子, 得到了一阶经典和量子微扰解. 特别是 我们的量子解在极限条件下能方便地转变为经典解, 并且坐标和动量算符的对易 关系的简化十分自然. 与Taylor级数解相比较, 无论是在经典还是在量子解 中频率移动都出现在各阶振动表达式中, 所以多尺度微扰解是弱耦合非简谐振动的较好解法.     

Quasilinearization method: Nonperturbative approach to physical problems

The general properties of the quasilinearization method (QLM), particularly its fast quadratic convergence, monotonicity, and numerical stability, are analyzed and illustrated on different physical problems. The method approaches the solution of a nonlinear differential equation by approximating the nonlinear terms by a sequence of linear ones and is not based on the existence of a small parameter. It is shown that QLM gives excellent results when applied to different nonlinear differential equations in physics, such as Blasius, Lane-Emden, and Thomas-Fermi equations, as well as in computation of ground and excited bound-state energies and wave functions in quantum mechanics (where it can be applied by casting the Schrödinger equation in the nonlinear Riccati form) for a variety of potentials most of which are not treatable with the help of perturbation theory. The convergence of the QLM expansion of both energies and wave functions for all states is very fast and the first few iterations already yield extremely precise results. The QLM approximations, unlike the asymptotic series in perturbation theory and 1/N expansions, are not divergent at higher orders. The method sums many orders of perturbation theory as well as of the WKB expansion. It provides final and accurate answers for large and infinite values of the coupling constants and is able to handle even supersingular potentials for which each term of the perturbation series is infinite and the perturbation expansion does not exist.     

单模激光系统输入信号后的稳态平均光强相对涨落

研究了具有实虚部间关联的量子噪声和抽运噪声驱动的单模激光系统输入信号后的统计性质,采用线性化近似方法计算了系统的稳态平均光强相对涨落,分析了量子噪声实虚部间关联系数、量子噪声强度、抽运噪声强度、输入信号振幅和频率、净增益等对稳态平均光强相对涨落的影响,发现在量子噪声实虚部间弱关联、小噪声、远离阚值、信号振幅不大和频率较高的条件下激光场的统计涨落较小。     

Generalized two phonon theory

Recent laser experiments and theoretical discussions of coherent two photon transient phenomena have prompted us to develop a generalized theory for the case of anN+2 level quantum system interacting with two optical fields. New perturbation solutions, derived from an effective two level Hamiltonian, are presented in the form of a continued fraction expansion where the leading term agrees with earlier treatments. The theory applies to homogeneously broadened systems where the intermediate transitions are far off resonance. When inhomogeneous broadening plays a role, the expansion parameter is no longer unique and the theory breaks down. Nonperturbative solutions are then required which are also capable of explaining other features not appearing in the perturbative approach. An important example is intensity-dependent dephasing. Exact and approximate solutions of this kind are derived.     

Dynamical Horizon Entropy Bound Conjecture in Loop Quantum Cosmology

The covariant entropy bound conjecture is an important hint for the quantum gravity, with several versions available in the literature. For cosmology, Ashtekar and Wilson-Ewing ever show the consistence between the loop gravity theory and one version of this conjecture. Recently, He and Zhang [J. High Energy Phys. 10 (2007) 077] proposed a version for the dynamical horizon of the universe, which validates the entropy bound conjecture for the cosmology filled with perfect fluid in the classical scenario when the universe is far away from the big bang singularity. However, their conjecture breaks down near big bang region. We examine this conjecture in the context of the loop quantum cosmology. With the example of photon gas, this conjecture is protected by the quantum geometry effects as expected.     

Dynamical Horizon Entropy Bound Conjecture in Loop Quantum Cosmology

The covariant entropy bound conjecture is an important hint for the quantum gravity, with several versions available in the literature. For cosmology, Ashtekar and Wilson-Ewing ever show the consistence between the loop gravity theory and one version of this conjecture. Recently, He and Zhang [J. High Energy Phys. 10 (2007) 077] proposed a version for the dynamical horizon of the universe, which validates the entropy bound conjecture for the cosmology filled with perfect fluid in the classical scenario when the universe is far away from the big bang singularity. However, their conjecture breaks down near big bang region. We examine this conjecture in the context of the loop quantum cosmology. With the example of photon gas, this conjecture is protected by the quantum geometry effects as expected.     

光纤中单光子传输方程的求解及分析

量子信息在光纤中传输时,会受到光纤损耗、色散、非线性效应等多因素的影响,将产生传输态的演化与能量转移.本文以单模光纤传输方程以及电磁场量子化理论为基础,对单模光纤中基模模场进行量子化处理,推导并建立了考虑损耗、色散、非线性效应后的单光子传输方程.基于微扰法对单光子非线性传输方程进行了求解,给出了稳定解存在的必要条件及其所满足的色散方程.深入讨论了广域光功率随微扰频率的变化关系,并且分析了光纤色散、非线性效应对解的影响.为量子光纤传输系统性能的深入研究奠定了理论基础.     

q形变光场与级联型三能级原子相互作用中场的压缩效应

建立了q形变光场与级联型三能级原子相互作用的非线性理论,求得相互作用绘景中薛定谔方程的形式解,利用数值计算讨论了q形变对相互作用中场压缩效应的影响并与q-偶相干光场的情形做了对比分析。研究发现,q偏离1的程度越大,q形变对场压缩效应的调控能力越强,反映出q形变的非线性行为对量子相干性的干扰以及对量子特性的影响。当q→1时,恢复为普通线性理论。和q-偶相干光场的情形做的对比分析,反映出q-奇相干光场不仅不存在压缩效应,还会弱化压缩效应。这与q-偶相干光场和q-奇相干光场存在不同的量子效应的结论完全一致。     

Photon higher-order squeezing effects of the q analogue of a single-mode field interacting with a Ξ-type three-level atom

The nonlinear theory of interaction between the q analogue of a single-mode field and a Ξ-type three-level atom has been established. And the formal solution of the Schrodinger equation in the representation and its average number are obtained. Then, the photon squeezing effects are studied through numerical calculation. The results show that the q deformation nonlinear action has a lot of influence on the quantum coherence and quantum properties. When q approaches 1, the theory reduces to the common linear theory.