SU(3)×SU(3) symmetry breaking, (8, 8) Model and theη→3π decay

It is shown that the (8, 8) model and explicitηπ ⁰ mixing successfully explain theη→3π decay width whereas the decay width calculated from the mass difference is about one order less than the experimental value.     

Total cross sections of electron scattering by molecules NF3, PF3, N(CH3)3, P(CH3)3, NH(CH3)2, PH(CH3)2, NH2CH3 and PH2CH3 at 30–5000 eV

Total cross sections of electron scattering by eight molecules NF₃, PF₃, N(CH₃)₃, P(CH₃)₃, NH(CH₃)₂, PH(CH₃)₂, NH₂CH₃ and PH₂CH₃, which have some structural similarities, are calculated at the Hartree-Fork level by the modified additivity rule approach [D.H. Shi, J.F. Sun, Z.L. Zhu, H. Ma, Y.F. Liu, Eur. Phys. J. D 45, 253 (2007); D.H. Shi, J.F. Sun, Y.F. Liu, Z.L. Zhu, X.D. Yang, Chin. Opt. Lett. 4, 192 (2006)]. The modified additivity rule approach takes into considerations that the contributions of the geometric shielding effect vary as the energy of incident electrons, the dimension of target molecule, the number of electrons in the molecule and the number of atoms constituting the molecule. The present investigations cover the impact energy range from 30 to 5000 eV. The quantitative total cross sections are compared with those obtained by experiments and other theories. Excellent agreement is observed even at energies of several tens of eV. It shows that the modified additivity rule approach is applicable to carry out the total cross section calculations of electron scattering by these molecules at intermediate and high energies, in particular over the energy range above 80 eV or so. It proves that the microscopic molecular properties, such as the geometrical size of the target and the number of atoms constituting the molecule, are of crucial importance in the TCS calculations. The new results for PH(CH₃)₂ and PH₂CH₃ are also presented at energies from 30 to 5000 eV, although no experimental and theoretical data are available for comparison. In the present calculations, the atoms are still represented by the spherical complex optical potential, which is composed of static, exchange, polarization and absorption terms.     

Critical (Φ4)3,ε

The Euclidean (⁴)_3, model in R³ corresponds to a perturbation by a ⁴ interaction of a Gaussian measure on scalar fields with a covariance depending on a real parameter in the range 01. For =1 one recovers the covariance of a massless scalar field in R³. For =0, ⁴ is a marginal interaction. For 0<1 the covariance continues to be Osterwalder-Schrader and pointwise positive. We consider the infinite volume critical theory with a fixed ultraviolet cutoff at the unit length scale and we prove that for >0, sufficiently small, there exists a non-gaussian fixed point (with one unstable direction) of the Renormalization Group iterations. We construct the stable critical manifold near this fixed point and prove that under Renormalization Group iterations the critical theories converge to the fixed point. Partially supported by NSERC of CanadaLaboratoire Associé au CNRS. UMR 5825Partially supported by CNR, G.N.F.M. and MURST     

M3La(BO3)3(M=Ca,Sr,Ba)基质中Eu3+的光致发光

研究了M3La(BO3)3(M=Ca,Sr,Ba)基质中Eu3+的激发光谱和发射光谱.结果表明,最强激发峰均为394nm,并均有λ<300nm的较强电荷迁移带;按Ca-Sr-Ba的顺序,各发射峰峰值逐渐红移;Eu3+的最佳发射浓度分别为xEu3+=0.10、0.09、0.20;Eu3+的5D0→7F2跃迁发射的浓度猝灭机理分别为电偶极-四极、电偶极-偶极和电偶极-偶极相互作用.     

(Pr,Nd)_(2/3)Sr_(1/3)MnO_3体系中的低温比热反常现象

主要研究了(Pr1-yNdy)2/3Sr1/3MnO3体系多晶样品在低温下的比热反常现象.Pr2/3Sr1/3MnO3在低温下没有比热反常现象,但随着Nd替代Pr,比热反常开始出现,峰值逐渐增加,峰值出现温度逐渐减小;在磁场的作用下,峰值减小,峰值出现温度逐渐增加;经分析,该低温比热反常现象与Schottky效应相关.     

Structural analysis of nonlinearities of Ca4ReO(BO3)3 (Re = La, Nd, Sm, Gd, Er, Y)

4 ReO(BO₃)₃ (CReOB, Re=La, Nd, Sm, Gd, Er, and Y) have been theoretically predicted. The d₁₁ tensor coefficient of CReOB is predicted to be -11 d₃₆(KDP), which is the largest d_ij tensor that has been found in borate crystals. From the structural characteristic of CReOB, we find the isolated BO₃ ^3- clusters play a dominant role in contributions to the total nonlinearity, and the largest d₁₁ tensor of CReOB-type crystals is also ascribed to these BO₃ ^3- clusters. We also find the NLO property of this family does not change dramatically for different rare-earth elements. The details of the calculation of CGdOB only are presented. Received: 3 March 1998/Accepted: 22 June 1998     

Electron spin resonance spectrum of radicals in γ-irradiated trimethyl phosphite: P(OMe)4, HP(OMe)3, P(OMe)2, (MeO)3P-P(OMe)3 + and H2COP(OMe)2

The infra-red spectra of 1 : 1 complexes between benzene and chlorine, bromine, and iodine chloride have been studied, with the complexes isolated in a nitrogen matrix at 20 K. The results are interpreted as evidence for an oblique complex structure, with the halogen molecule interacting mainly with one of the C=C bonds.     

Eu_(0.9)M_(0.1)TiO_3(M=Ca,Sr,Ba,La,Ce,Sm)的磁性和磁热效应

EuTi0_3是直接带隙半导体材料,在液氦温度附近呈现反铁磁性,且具有较大的磁熵变,但是当其转变为铁磁性时,可以有效提高低磁场下的磁熵变.本文通过元素替代,研究晶格常数的变化和电子掺杂对磁性和磁热效应的影响.实验采用溶胶凝胶法制备EuTiO_3和Eu_(0.9)M_(0.1)TiO_3 (M=Ca, Sr, Ba, La, Ce, Sm)系列样品.结果表明:大离子半径的碱土金属离子替代提高了铁磁性耦合,有利于提高低磁场下的磁热效应.电子掺杂可以抑制其反铁磁性耦合从而使其表现为铁磁性.当大离子半径的稀土La和Ce离子替代Eu离子时,既增大了晶格常数也实现了电子掺杂,表现出较强的铁磁性.在1 T的磁场变化下,Eu_(0.9)La_(0.1)TiO_3和Eu_(0.9)Ce_(0.1)TiO_3的最大磁熵变分别为10.8和11 J/(kg·K),均大于EuTi0_3的9.8 J/(kg·K);制冷能力分别为39.3和51.8 J/kg,相对于EuTi0_3也有所提高.     

Dy~(3+),Sm~(3+)和Ce~(3+)离子在M_3La_2(BO_3)_4(M=Ca,Sr,Ba)中光谱性质的研究

本文报导了Dy~(3+),Sm~(3+)和Ce~(3+)离子在M_3La_2(BO_3)_4(M=Ca,Sr,Ba)基质中的激发与发射光谱;研究了Dy~(3+)离子黄蓝发射的相强度随基质化合物的组成和结构的不同而呈现的变化规律;讨论了Sm~(3+)离子电荷迁移激发带的能量与基质中近邻阳离子的关系并分析了Sm~(3+)和Eu~(3+)离子4f电子构型对电荷迁移带能量的影响。本文还给出了Dy~(3+),Sm~(3+)和Ce~(3+)离子发光的浓度淬灭值。     

LnAlO_3中Ce~(3+),Tb~(3+),Dy~(3+)的发光及Ce-Tb,Ce-Dy的敏化发光(Ln=La,Gd,Y)

本文采用BaF_2作为助熔剂和抑制剂经固相反应合成了一系列以LnAlO_3(Ln=La,Gd,Y)为基质的磷光体,系统地研究了LnAlO_3中Ce~(3+),Tb~(3+),Dy~(3+)的发光及Ce-Tb,Ce-Dy的敏化发光,发现随Ln的不同,LnAlO_3作为基质对激活剂的发光性质的影响也不同,本文得到一些规律性结果,并作了讨论。     

(n,3He)的反应截面的系统学

本文研究了中、重质量核的14MeV中子的(n,~3He)反应截面的系统学特性,在对实验数据分析,评价的基础上,给出了系统学的经验公式,计算了一批核素的反应截面,同实验值符合较好,并讨论了可能的反应机制。 The systematic characters of (n, ~3He) reaction cross sections have been studied formedium and heavy mass nucleus at 14MeV. A set of the empirital parameters have been eatracted onthe bases of analyzing and evaluating available data. The (n,~3He) reaction cross sections of somenuclei have been calculated, and a good agreement with the experimental data have been obtained.Most possible reaction mechanisms are also discussed.     

(Y,Gd)Al3(BO3)4:Tb的真空紫外光谱特性

(Y,Gd)Al3(BO3)4属于三角晶系,具有R32的空间群,掺入Ce3 ,Tb3 杂质后,其晶格结构没有变化。(Y,Gd)Al3(BO3)4:Tb随着Gd3 摩尔浓度增大,基质吸收带红移。Gd3 和Tb3 之间存在着很有效的能量传递。Gd3 摩尔浓度在一定范围内(0~0·75mol)增大时,样品在120~300nm光谱范围内的激发强度均是增强的;但是,Gd3 浓度过高造成Gd3 的发射增强,GdAl3(BO3)4:Tb在120~240nm光谱范围内激发强度很明显下降。(Y,Gd)Al3(BO3)4:Ce,Tb在真空紫外激发下,发现Tb3 的发光明显的被Ce3 猝灭。     

195Pt,15N NMR spectroscopy of aqueous solutions of mixed valent oxonitrocomplexes,Pt(II,IV): K5[(NO2)3PtIV(μ-O)3 Pt 3 II (NO2)6] and K8[(NO2)6Pt 3 II (μ-O)3PtIV(μ-O)3Pt 3 II (NO2)6]

Two aqueous solutions of oxonitrocomplexes comprising di- and tetravalent platinum atoms, K₅[(NO₂)₃Pt^IV(μ-O)₃Pt ₃ ^II (NO₂)₆]· 3H₂O and K₈[(NO₂)₆Pt ₃ ^II (μ-O)₃Pt^IV (μ-O)₃Pt ₃ ^II (NO₂)₆] · 7H₂O, have been studied by¹⁹⁵Pt and¹⁵N NMR technique. Both compounds, enriched with the¹⁵N (95%) isotope, were synthesized by thermal denitrozylation of K₂[Pt(NO₂)₄]. Constants of spin-spin scalar coupling,¹⁹⁵Pt-¹⁵N and¹⁹⁵Pt^II-¹⁹⁵Pt^IV, were obtained for tetra-and heptameric complexes in aqueous solutions through multiplet simulation. The¹⁹⁵Pt and¹⁵N NMR spectra of the same solutions obtained two months after their preparation show signals from the hydrolytic forms of the tetrameric complex as well as the signals from mono- di- and trimeric oxonitrocomplex forms of divalent platinum. All signals of species formed as a result of hydrolysis were identified.     

Cr3+:GGG(Ca,Mg,Zr)和Nd3+,Cr3+:GGG(Ca,Mg,Zr)激光晶体的光谱特性

本文分析了Cr3+:GGG(Ca,Mg,Zr)的荧光谱和吸收谱,测算到Cr3+离子在4T2g-2Eg的能级间距为ΔE≈70cm-1,晶场强度Dq/B=2.50.说明由于GGGa(Ca,Mg,Zr)晶格扩大减弱了晶场,可望实现Cr3+:GGG(Ca,Mg,Zr)室温下的调谐及Nd3+:Cr3+:GGG(Ca,Mg,Zr)中Cr3+→Nd3+能量的转移.最后从理论上阐明了Cr3+在晶体GGG(Ca,Mg,Zr)中的能级结构.     

YbPO_4基质中Yb~(3 )-Yb~(3 )和Yb~(3 )-Gd~(3 )离子对的合作光学跃迁

研究了YbPO_4基质中Yb~(3 )-Yb~(3 )和Yb~(3 )-Gd~(3 )离子对的三种类型的合作光学跃迁,即合作吸收,合作发光,以及喇曼发光,在这些现象中,跃迁谱线的能量与所予期的单个离子的跃迁能量相当一致在YbPO_4的点群对称D_(2d)的晶体场下,Yb~(3 )离子的两个4f多重项~2F_(7/2)和~2F_(5/2),大约相隔10,000cm~(-1),应是分别劈裂成四个和三个能级。这些晶体场-劈裂能级的能量从YbPO_4单晶的吸收和发射光谱得到。     

掺Ce3+、Tb3+的M3Y2(BO3)4(M＝Ca,Sr)

采用固相反应的方法;经二次灼烧合成了掺Ce3+、Tb3+的Ca3Y2(BO3)4和Sr3Y2(BO3)4磷光体;分析了合成过程中铈的还原情况.用X-射线衍射分析确定了它们的结构均为正交晶系,空间群P21cn测定了Ce3+和Tb3+在两种基质中的光谱,得到Ce3+波长位移的某些规律,观察到Ce3+对Tb3+的敏化作用.     

The 3He(α, γ)7Be and 3He(α, γ)7Li reactions at astrophysical energies

The radiative capture cross sections for ³He(α, γ)⁷Be and ³He(α, γ)⁷Li at astrophysical energies have been studied microscopically in terms of the resonating group method. It was found that the astrophysical S-factors correlate strongly to the nuclear size and deformation of ⁷Be and ⁷Li. With the help of measured nuclear properties of these nuclei, a safety range of the absolute values of the S-factor was determined; the most recommended S(0)-values are 0.50 ± 0.03 keV · b for the ³He(α, γ)⁷Be reaction and 0.098 ± 0.006 keV · b for the ³H(α, γ)⁷Li reaction.     

Photoluminescence properties of Y_(0.75-x)Gd_xAl_(0.10)BO_3:Eu_(0.10)~(3+),0.05R~(3+)(R= Sc,Bi) (0.00 ≤ x ≤ 0.45)

Y 0.75 -x Gd x Al 0.10 BO 3 :Eu0.10 3+, 0.05R 3+ (R=Sc, Bi) (0.00 ≤ x ≤ 0.45) powder samples are prepared by solid-state reaction and their luminescence properties are investigated. With the replacement of Y 3+ ions by Sc 3+ (or Bi 3+ ) and Gd 3+ ions in (Y,Al)BO 3 :Eu, the intensities of emission at 254 and 147 nm are remarkably improved, because Sc 3+ ions can absorb UV light and transfer the energy to Eu 3+ ions efficiently. Moreover, Gd 3+ and Bi 3+ ions act as an intermediate "bridge" between the sensitizer and the activator (Eu 3+ ) in energy transfer to produce light in the (Y, Gd)BO 3 :Bi 3+ , Eu 3+ system more effectively. After doping an appropriate concentration of Gd 3+ into Y 0.50 Gd 0.25 Al 0.10 BO 3 :Eu0.01 3+ , Bi0.05 3+ , the emission intensity reaches its maximum, which is nearly 110% compared with the red commercial phosphor (Y,Gd)BO 3 :Eu and better chromaticity coordinates (0.650, 0.350) are obtained.     

Nuclear structure studies of 125Te with (n,γ), (d,p) and (3He,α) reactions

Levels in ¹²⁵Te were investigated in the range up to 3.3 MeV excitation energy by the (n,γ), (d,p) and (³He,α) reactions. Over 160 levels and about 360 γ-transitions were established, most for the first time. The states below 2.3 MeV with the most complete spectroscopic information were interpreted in terms of the interacting boson-fermion model (IBFM). Unitary treatment of both positive- and negative-parity states is achieved with the same model parameter close to the intermediate case between O(6) and U(5) limits. Excitation energies, electromagnetic transition rates, γ-branchings and spectroscopic factors are discussed in connection with the possible structures. A family of low-spin negative-parity states has been identified and understood by the IBFM proving their antialigned origin.