关于B.W.Lee的公式Г*Г=0的推广

本文将B.W.Lee的公式Г*Г=0推广为Г~(AF)＊Г~(AF)=0,只要命B.W.Lee公式中的dλ=ζ_1ζ_2ζ_0即可,而不需要B.W.Lee式的二次变化等于零的限制。从而,该公式不仅包含了B.W.Lee的公式,而且能直接解决其他一些问题。     

SU(2)×U(1)×S3模型及类K0-K0系统的混合和CP破坏效应

本文内容包括:(ⅰ)进一步给出SU(2)×U(1)×S₃模型的结果S₂≈S₃≈(m_s²)/(m_b²);sin δ≤(m_um_d)/(m_cm_s),并预言b夸克的主要衰变道是b→u+W,b夸克的寿命可能长到10^-9秒.(ⅱ)给出类K⁰-K⁰系统混合时的精确表达式ρ=错号事例数/对号事例数=(1/2)(|p/q|²+|q/p|²)([Γ²+(Δm)²]²-(γ1γ2)²)/([Γ²+(Δm)²]²+(γ1γ2)²);并给出CP破坏的精确表达式:A=(1-ρ')/(1+ρ')=(I_M12Γ₁₂^*)/(|M₁₂|²+1/4|Γ₁₂|²),这里ρ′=(负电错号事例数)/(正电错号事例数)。     

不等质量(1/2—1/2)或(1/2-1/2)电磁束缚系统的近似B.S.波函数

本文求解了不等质量(1/2—1/2)电磁束缚系统的Bethe-Salpeter方程. 给出了这类系统的近似B.S.波函数. 利用复合粒子量子场论的微扰展开, 在精确到O(α)的量级下, 计算了Ξ⁰→(Σ⁺μ^－)+ν_μ的衰变率和分支比, 结果是wΞ⁰→(Σ⁺μ^－)+ν_μ=1.12(1/秒)R=[wΞ⁰→(Σ⁺μ^－)+ν_μ]/[wΞ⁰→(Σ⁺μ^－)+ν_μ]≥4.7×10^－7. 类似地, 还讨论了Λ→(pμ^－)+ν_μ过程.     

用3+1维理论计算强子的1—0衰变过程

本文在Krapchev's L₀近似下, 用3+1维理论讨论强子的1—0衰变过程, 计算了耦合常数f_π, 电磁衰变宽度ΓV→l⁺l^－等. 在计算过程中, 不象文献[1]那样引入唯象因子Vbag, 但所得结果较好地符合于实验.     

31.2MeV α粒子在B核上的(α,t)、(α,d)和(α,p)反应的研究

我们用粒子鉴别系统测量了31.2MeV的α粒子在^11,10B核上的(α,t)、(α,d)和(α,p)反应的角分布; 由出射粒子的能谱, 我们分别得到了剩余核处于基态和不同激发态的十个角分布. 从角分布的形状看, 在¹¹B(α,t₀)¹²C_g﹒s, ¹¹B(α,d₀)¹³C_g﹒s, ¹⁰B(α,d₀)¹²C_g﹒s, ¹⁰B(α,d₁)¹²C_1st, ¹¹B(α,p₀)¹⁴C_g﹒s等反应中均有不同程度的后角上翘; 并且(α,t₀)和(α,p₀)的后角上翘的同位素效应似乎与(α, α)的反常散射的同位素效应相反.     

Kerr-Newman度规中带电Bose子束缚态

本文指出, 无质量Bose子和Kerr-Newman黑洞不形成束缚态. 有质量的Bose子, 在0<α<√M²－Q²的情况下, 若E≠am+eQr₊/2Mr₊－Q²则无束缚态; 若E=am+eQr₊/2Mr₊－Q²则非束缚态存在的必要条件是(22)和(24)式. 在a=√M²－Q²的情况, 束缚态的能量E=√M²－Q²+eQM/2M²－Q², 当Q=0或者e=0时, 本文结论与de Felic^[1]和章世伟、苏汝铿^[2]的结果相符.     

12C离子与各种靶核相互作用的裂变激发函数

本工作采用金硅面垒型半导体探测器和固体径迹探测器测量了57.0—73.0MeV ¹²C+¹⁶⁹Tm, ¹⁷⁵Lu, ¹⁸¹Ta, W, Re, Pt, ¹⁹⁷Au, Pb和²⁰⁹Bi裂变反应碎片角分布和裂变激发函数. 由相当于全动量转移的裂变事件的碎片角分布统计理论直接确定了全熔合反应截面σ_fu, 从而获得了作为激发能函数的<Γ_f/Γ_n>实验值. 与理论计算符合得到裂变位垒高度, 标准偏差为2.5MeV. 实验上确定的裂变位垒与非旋转液滴模型计算值相符合. 用同样方法, 我们还分析了已经发表了的¹²C+¹⁷⁴Yb, ¹²C+¹⁹⁸Pt, ¹⁶O+¹⁴²Nd, ¹⁶O+¹⁷⁰Er, ¹⁶O+¹⁸¹Ta和¹⁸O+¹⁹²Os裂变反应激发函数, 研究了裂变位垒随裂变核质量数A的变化, 并且和液滴模型理论做了比较.     

在K0-K0系统理论中的一个重要问题

利用对K⁰-K⁰系统相位无关的描写公式, 讨论了在计算M₁₂时的B参量的符号及K-M矩阵中sin δ的符号(都应大于零). 也讨论了精确的ε表达式中的奇异性的意义. 这个奇异性在文献中常见的公式里不存在.     

Testing lepton flavor universality in terms of BESⅢ and charm-tau factory data

The recent measurements on R_K and R_π imply that there exists a possible violation of the leptonic flavor universality which is one of the cornerstones of the Standard Model. It is suggested that a mixing between sterile and active neutrinos might induce such a violation. In this work we consider the scenarios with one or two sterile neutrinos to explicitly realize the data while the constraints from the available experiments have been taken into account. Moreover, as indicated in literature, the deviation of the real PMNS matrix from the symmetric patterns may be due to a μ-τ asymmetry, therefore the measurements on R_D(Ds)eμ=Γ(D(D_s)→ e⁺ν_e)/Γ(D(D_s)→ μ⁺ν_μ) and R_D(Ds)μτ=Γ(D(D_s)→ μ⁺ν_μ)/Γ(D(D_s)→ τ⁺ν_τ) (and for some other heavy mesons B^± and B_c etc.) may shed more light on the physics responsible for the violation of the leptonic flavor universality. The data of BESⅢ are available to test the universality and that of future charm-tau factories will provide more accurate information. In this work, we will discuss R_D(Ds)eμ and R_D(Ds)μτ in detail and also briefly consider the cases for B^± and B_c.     

对带电轻子质量公式的一些猜测

本文建议轻子电磁自能通过（（δm）/m）=（1/（2π））n^-b 与量子数 n 联系起来,其中 b 为待定常数.并建议动量截断值 M 与引力常数 k 和精细结构常数α的联系为 M=（?）.得到了带电轻子质量公式（?）.利用 e^-和μ^-质量的实验值和α值作输入,给出计算值 k=（6.67231±0.00026）×10^-8 cm³g^-lsec^-2和m_τ=（1782.306±0.078）MeV,与观察值 k=（6.6720±0.0041）×10^-8cm³ g^-1sec^-2和 m_τ=(1782_-4⁺³)MeV 很好符合.公式预言第四个带电轻子质量应为 m=（11725.47±0.51）MeV 可以在最近的实验中检验。本文还对所建议的质量公式和结果进行了讨论.     

Study of pure annihilation decays Bd,s→D0D0

Within the heavy quark limit and the hierarchy approximation λ_QCD<< m_D<B, we analyze the B→D⁰D⁰ and B_s→D⁰D⁰ decays, which occur purely via annihilation type diagrams. As a rough estimate, we calculate their branching ratios and CP asymmetries in the perturbative QCD (PQCD) approach. The branching ratio of B→D⁰D⁰ is about 3.8×10^－5 that is just below the latest experimental upper limit. The branching ratio of B_s→D⁰D⁰ is about 6.8×10^－4, which could be measured in LHC-b. From the calculation, it is found that this branching ratio is not sensitive to the weak phase angle γ. In these two decay modes, there exist CP asymmetries because of the interference between weak and strong interaction. However, these asymmetries are too small to be measured easily.     

Fourth generation effects in Bs→π^-K^＋ decay

We study the effects of the fourth quark generation model in B_s → π^-K⁺ decay. Combining with the up-to-date experimental measurement for B(B_s → π^-K⁺) and A_cp^dir(B_s → π^-K⁺) by the CDF Collaboration, we derive the new bound of weak phase ø_bd, which are 0°< ø_bd <44°, 321°< ø_bd < 360° and 0°< ø_bd < 26°, 342°< ø_bd < 360° for m_t'=400 and 600 GeV respectively. In these regions, B(B_s → π^-K⁺) and A_cp^dir(B_s → π^-K⁺) consist with the current experimental data within errors.     

Description of the evolution of mixed-symmetry states in the N=78 isotonic chain with IBM2

The characteristics of the lowest mixed-symmetry states 2_ms⁺ and 1_ms⁺ for ¹³²Xe, ¹³⁴Ba and ¹³⁶Ce in the even-even N=78 isotones are investigated within the framework of the IBM2 model. The lowest mixed-symmetry state 2_ms⁺ levels for both a single isolated state in ¹³²Xe and ¹³⁶Ce and a fragmented state in ¹³⁴Ba are reproduced by the predictions. The agreement between the IBM2 calculation and the experimental values is good for the B(E2) and B(M1) transition probabilities both quantitatively and qualitatively. The predicted summed B(M1) strength follows the experimental data, remaining nearly constant as a function of proton number along the chain of the N=78 isotones.     

B离子对SiO2基质凝胶中Eu3+特征光谱的加强作用

使用正硅酸乙酯、硼酸和硝酸铝为前驱体，硝酸铕为掺杂剂，以溶胶-凝胶法制备了Eu单掺和Eu、B共掺的SiO2干凝胶，并成功地在钠钙玻璃上制备了光洁度很好的掺杂SiO₂多层薄膜.利用荧光光谱、红外光谱（IR）、X射线衍射（XRD）等技术研究了B离子、退火温度对样品发光性能的影响.荧光光谱显示发光体能产生很强的红色发光，经500℃以上退火处理，产生6条谱带，分别归属于Eu³⁺的⁵D₀→⁷F_J（J=0, 1, 2, 3, 4）的电子跃迁, ⁵D₀→⁷F₁的跃迁分裂为两个峰.实验结果表明，B离子的加入，由于在材料中形成了Si-O-B键，使Eu³⁺的配位环境的对称性降低，加强了Eu³⁺的红光发射.退火处理改变了材料的网络结构，降低了水和羟基的含量有助于提高发光强度，但退火温度太高（850℃），发生了荧光猝灭效应，源于稀土离子发生位置迁移形成的团簇.XRD测试结果显示材料是非晶态的.     

对爱因斯坦模型的修正及考虑热效应的三个通用状态方程

 对固体考虑热效应的爱因斯坦模型进行了修正。指出考虑热效应的通用状态方程中不应该包含零点振动项，方程参数不应该直接取为参考温度下的实验值V_R，B_R，B′_R和γ^G_R，而应该取为零温下的数值V₀，B₀，B′₀和γ^G₀；提出了一种从V_R，B_R，B′_R和γ^G_R求解V₀，B₀，B′₀和γ^G₀的方法。将提出的方法应用于三个典型的通用状态方程，包括Baonza、mMNH和Vinet方程。数值结果表明，利用相同的实验参数对三个方程解出的参数，以及预测的零压和低压下的热物理性质差异很小，而且都与实验数据符合很好。这些结果表明，在零压和低压下预测热物理性质的精确度不足以用来判断各种通用状态方程的适用性。     

Evidence for e+e-→γχc1,2 at center-of-mass energies from 4.009 to 4.360 GeV

Using data samples collected at center-of-mass energies of √s=4.009, 4.230, 4.260, and 4.360 GeV with the BES0 detector operating at the BEPC/ collider, we perform a search for the process e⁺e^-→γχ_c,j (J =0, 1, 2) and find evidence for e⁺e^-→γχ_c1 and e⁺e^-→γχ_c2 with statistical significances of 3.0σ and 3.4σ, respectively. The Born cross sections σ^B(e⁺e^-→γχ_c,j), as well as their upper limits at the 90% con dence level (C.L.) are determined at each center-of-mass energy.     

e-1<（压缩因子Z）

 从正则系综的基本公式出发，绕开对位形积分的具体计算，结合热力学能态方程，求出了e^-1<压缩因子Z0, p₀)附近压力与温度的一般解析式，并与实验值进行了对照。应用本文导出的公式在工程热物理方面可减少实验测试的次数，在石化工业中可用来计算环境温度的变化对高压储气罐内压力的影响。     

Electromagnetic transition properties and isospin excitation in the cross-conjugate nuclei 44Ti and 52Fe

The interacting boson model with isospin (IBM-3) is applied to study the band structure and electromagnetic transition properties of the low-lying states in the cross-conjugate nuclei ⁴⁴Ti and ⁵²Fe. The isospin excitation states with T=0, 1 and 2 are identified and compared with available data. The E2 and M1 matrix elements for the low-lying states have been investigated. According to this study, the 2₃⁺ state is the lowest mixed symmetry state in the cross-conjugate nuclei ⁴⁴Ti and ⁵²Fe. The excitation energy of the second 0₂⁺ and 2₂⁺ states with T=0 in the nucleus ⁵²Fe are identified. The agreement between the model calculations and data is reasonably good.     

费米子数的时空性质

将4维 Minkowski 时空推广到5维时空,并将“基本”粒子静质量和时空自由度 x₅相联系,m=—i（（?）/（?）x₅）,我们讨论了5维非线性变换共形群 C（M₅）.对于C（M₅）交换,保持有 dx₁²+dx₂²+dx₃²-dx₀²+dx₅²=0不变.C（M₅）群和线性变换群 SO（5,2）同构.在此基础上我们分析了费米子数的时空性质,并给出了自旋为半整数（整数）的粒子费米子数为奇数（偶数）的这一实验规律.     

压力对GdoBr:Eu晶场参数的影响

 在室温下测量了GdoBr:Eu的常压和高压荧光谱，光谱范围在13 000~21 500 cm^-1之间，压力至12 GPa。由光谱数据得到了Eu³⁺晶场能级随压力的变化曲线。⁷F_0～5能级随压力的变化规律比较复杂，而⁵D_0~2各能均随压力的升高几乎线性地降低。在基态谱项⁷F的49个状态上进行了晶场拟合计算，所得常压下的5个非零晶场参数分别为：B₀²＝-1 124.0 cm^-1，B₀⁴＝-969.6 cm^-1，B₄⁴＝827.9 cm^-1，B₀⁶＝889.6 cm^-1，B₄⁶＝377.0 cm^-1。高压下的计算结果表明，B₀⁴、B₀⁶这两个晶场参数随压力的增加而增大，B₄⁶随压力的增加而减小，而B₀²、B₄⁴随压力的变化有些起伏。晶场强度在8 GPa以下随压力增加而减小，其后开始变强。