约束力学系统的联络及其运动方程的测地性质

用现代整体微分几何方法研究非定常约束力学系统运动方程的测地性质，得到非定常力学系统的动力学流关于１＿射丛上的联络具有测地性质的充分必要条件·非定常情形下的动力学流关于无挠率的联络总具有测地性质，因此任何非定常约束力学系统在外力作用下的运动总可以表示为关于１＿射丛上无挠率的动力学联络的测地运动，这与定常力学的情形有所区别·     

A U（4） QCD Model Using Generalized Yang-Mills Theory

Generalized Yang-Mills theory has a covariant derivative which contains both vector and pseudoscalar gauge bosons. Based on this theory, we construct a U（4） strong interaction model. By using this U（4） generalized Yang-Mills model, we obtain that mesons can be realized as the colorless pseudoscalar gauge bosons. We also obtain a gauge potential solution which can be used to explain the asymptotic behavior and color confinement.     

A Representation of the Lorentz Spin Group and Its Application

For an integer m ≥ 4, we define a set of 2[m/2] × 2[m/2] matrices γj （m）, （j = 0, 1,..., m - 1） which satisfy γj （m）γk （m） ＋γk （m）γj （m） = 2ηjk （m）I[m/2], where （ηjk （m）） 0≤j,k≤m-1 is a diagonal matrix, the first diagonal element of which is 1 and the others are -1, I[m/2] is a 2[m/1] × 2[m/2] identity matrix with [m/2] being the integer part of m/2. For m = 4 and 5, the representation （m） of the Lorentz Spin group is known. For m≥ 6, we prove that （i） when m = 2n, （n ≥ 3）, （m） is the group generated by the set of matrices {T｜T=1/√ξ（（I＋k） 0 ＋ 0 I-K） （ U 0 0 U）, （ii） when m = 2n ＋ 1 （n≥ 3）, （m） is generated by the set of matrices {T｜T=1/√ξ（I -k^- k I）U,U∈ （m-1）,ξ=1-m-2 ∑k,j=0 ηkja^k a^j〉0, K=i[m-3 ∑j=0 a^j γj（m-2）＋a^（m-2） In],K^-=i[m-3∑j=0 a^j γj（m-2）-a^（m-2） In]}     

On Möbius form and Möbius isoparametric hypersurfaces

An umbilic-free hypersurface in the unit sphere is called MSbius isoparametric if it satisfies two conditions, namely, it has vanishing MSbius form and has constant MSbius principal curvatures. In this paper, under the condition of having constant MSbius principal curvatures, we show that the hypersurface is of vanishing MSbius form if and only if its MSbius form is parallel with respect to the Levi-Civita connection of its MSbius metric. Moreover, typical examples are constructed to show that the condition of having constant MSbius principal curvatures and that of having vanishing MSbius form are independent of each other.     

平行三次形式的仿射超曲面

设Ａｎ 1是ｎ 1维仿射空间 ,Ｄ表示Ａｎ 1上的平坦联络 ,Ｍ是ｎ维光滑流形 ,ｘ:Ｍ→Ａｎ 1是一个非退化的仿射浸入 .对于Ｍ上的横截向量场ξ ,存在唯一的选择 ξ =1ｎ△ｘ(称为仿射法向量场 ) ,使得上述浸入是一个Ｂｌａｓｃｈｋｅ浸入 (见 [2 ]) .设 是此浸入由Ｄ在Ｍ上诱导的仿射联络 ,我们有 :ＤＸＹ= ＸＹ ｈ(Ｘ ,Ｙ) ξ　　　ＤＸξ=-ＳＸ这里Ｘ ,Ｙ ,Ｚ是Ｍ上的切向量场 ,ｈ是对称的双线性形式 ,由它可以定义Ｍ上的伪黎曼度量Ｇ(Ｇ =|Ｈ| - 1ｎ 2 ｈ ,Ｈ =ｄｅｔ(ｈｉｊ) ) ,称为Ｂｌａｓｃｈｋｅ度量 ,Ｓ称为Ｍ的形态算子 .若…     

A QCD Model Using Generalized Yang-Mills Theory

Generalized Yang-Mills theory has a covariant derivative, which contains both vector and scalar gauge bosons. Based on this theory, we construct a strong interaction model by using the group U（4）. By using this U（4） generalized Yang-Mills model, we also obtain a gauge potential solution, which can be used to explain the asymptotic behavior and color confinement.     

射影半对称联络的一个不变量

本文研究与Levi-Civita联络▽射影等价地射影半对称联络D。获得了一个射影不变量,并给出其成立的一个充分必要条件。进而给出其保持相应共变导数不变的另一充分条件。     

滨海软土地层机械法联络通道施工影响监测分析

机械法联络通道T接施工技术是一种施工软土地区地铁联络通道的新型工法, 具有全程机械化、施工周期短、可直接切削主隧道和洞口等优点. 以宁波地铁3号线某联络通道工程为研究对象, 通过监测分析研究新工法对周围地层、主隧道结构等的施工影响. 结果表明: 受交叉施工影响, 联络通道纵向靠近主隧道的地表沉降较大, 靠近联络通道中央影响较小; 横向中心位置地表沉降较大, 两侧影响较小; 主隧道结构沉降及隧道断面收敛变形较小; 顶推过程对周围地层影响明显, 但水平地面受影响较小, 表明地层总体沉降量小, 基本可控. 此外, 采用peck曲线和高斯曲线分别描述纵横向地面沉降的变化特征, 采用回归分析确定了沉降曲线参数, 与实际监测结果相比, 两者拟合良好.     

Berry联络与吴－杨单极势

通过研究一半整数自旋值的中性粒子在球对称磁场中的Ｂｏｒｎ－Ｏｐｐｅｎｈｅｉｍｅｒ方程，发现在自旋空间Ｂｅｒｒｙ联络呈非阿贝尔形式．在绝热近似下，Ｂｅｒｒｙ联络相当于阿贝尔形式的吴－杨单极场．由于拓扑的非平庸性，利用纤维丛中截面的概念研究了位形空间的动力学，发现中心势场中粒子的角动量和能量均取量子化值，但数值发生移动，这是纯几何起源的现象．     

Dark Energy Coupled with Dark Matter in the Accelerating Universe

To model the observed Universe containing both dark energy and dark matter, we study the effective Yang-Mills condensate model of dark energy and add a non-relativistic matter component as the dark matter, which is generated out of the decaying dark energy at a constant rate Г, a parameter of our model. For the Universe driven by these two components, the dynamic evolution still has asymptotic behaviour: the expansion of the Universe is accelerating with an asymptotically constant rate H, and the densities of both components approach to finite constant values. Moreover, Ω△～ 0.7 for dark energy and Ωm～0.3 for dark matter are achieved if the decay rate Г is chosen such that Г/H ～ 1.