Er~(3+)离子浓度对ZnS:ErF_3薄膜交流电致发光特性的影响

本文研究了Er~(3+)离子浓度对ZnS:ErF_3薄膜交流电致发光(ACEL)特性的影响。I(~4F_(9/2)→~4I_(15/2))受Er~(3+)离子浓度的影响较大,随Er~(3+)离子浓度增高,I(~4F_(9/2)→~4I_(15/2))增强,甚至超过I(~2H_(11/2)→~4I_(15/2))。通过研究具有不同Er~(3+)离子浓度样品的电致发光衰减,绿红比随外加电压的变化关系以及不同能级的电致发光效率,我们发现,粒子从~4S_(3/2)和~2H_(11/2)能级向~4F_(9/2)能级弛豫是使I(~4F_(9/2)→~4I_(15/2))增强的主要原因。随Er~(3+)离子浓度增高,交叉弛豫速率也增高,因而使I(~4F_(9/2)→~4I_(15/2))随浓度的增高而增强。     

Er3+单掺、Er3+/Yb3+共掺杂Ca12Al14O32F2的 制备及上转换发光性质

利用高温固相法成功制备了Er~(3+)单掺、Er~(3+)/Yb~(3+)共掺杂Ca_(12)Al_(14)O_(32)F_2上转换发光样品。在980 nm激光激发下,Er~(3+)单掺和Er~(3+)/Yb~(3+)共掺杂样品均呈现出较强的绿光(528,549 nm)和较弱的红光(655 nm)发射,分别归因于Er~(3+)离子的~2H_(11/2),~4S_(3/2)→~4I_(15/2)和~4F_(9/2)→~4I_(15/2)能级跃迁。随着Er离子浓度的增加,单掺杂样品上转换发光强度先增大后减小,最佳掺杂浓度为0.8%。共掺杂Yb~(3+)后,Er~(3+)的发光强度明显增大。还原气氛下合成的样品上转换发光强度增大约两倍,可能和笼中阴离子基团变化有关。发光强度和激发光功率的关系表明所得上转换发射为双光子吸收过程,借助Er~(3+)-Yb~(3+)体系能级结构详细讨论了上转换发射的跃迁机制。     

Sc_2(WO_4)_3∶Er~(3+)/Yb~(3+)的上转换发光及其温度传感特性

通过高温固相法制备出一系列新型上转换材料Sc_2(WO_4)_3∶Er~(3+)/Yb~(3+)。在980 nm激光激发下,Sc_2(WO_4)_3∶Er~(3+)/Yb~(3+)样品发出肉眼可见的强绿光。利用荧光光度计测得样品的发光光谱,在500～600 nm之间有强绿光发射,分别归因于Er~(3+)的~2H_(11/2)→~4I_(15/2)和~4S_(3/2)→~4I_(15/2)跃迁发射。在650～700 nm位置处,有对应于Er~(3+)离子~4F_(9/2)→~4I_(15/2)跃迁的较弱的红光发射。随着掺杂浓度的变化,样品的红绿分支比发生变化。当样品掺杂Er~(3+)浓度为0.05%、Yb~(3+)浓度等于0.1%时,样品发射的绿光强度是红光强度的27倍。另外,利用荧光强度比方法研究了Er~(3+)的两个热耦合能级在303～573 K范围内的发光温度特性。393 K时,样品的灵敏度达到最大为0.006 8 K~(-1)。对比于其他荧光粉材料,Sc_2(WO_4)_3∶Er~(3+)/Yb~(3+)的灵敏度处于较高水平,在实际测温中具有更好的应用前景。     

Er~(3+)掺杂Na_5Lu_9F_(32)单晶体的红外光学特性

采用坩埚下降法成功地生长了Er~(3+)离子掺杂的Na_5Lu_9F_(32)(NLF)单晶体。测定了单晶体在400~2 500nm波段的吸收光谱与2.5~25μm红外波段的透过光谱。Na_5Lu_9F_(32)单晶体在400~7 150 nm宽波段范围具有好的光学透过性,在该波段的透过率达到90%。在透过光谱中几乎观察不到2.7μm中红外波段的吸收,说明单晶体中OH~-离子的含量极低。根据测定的吸收光谱,通过Judd-Ofelt理论计算了Er~(3+)在单晶体中的光学强度参数Ω_t(Ω_2=2.08,Ω_4=2.07,Ω_6=0.75),以及相应的辐射跃迁速率、荧光分支比和荧光寿命。根据Futchbauer-Ladenburg公式估算了样品的发射截面大约分别为1.42×10~(-20)cm~2(~4I_(13/2)→~4I_(15/2))和1.66×10~(-20)cm~2(~4I_(11/2)→~4I_(13/2))。在980 nm半导体激光器(LD)激发下,研究了单晶体的近红外1.5μm与中红外2.7μm的发射光谱特性。     

银表面等离子体对掺铒铋化物发光玻璃中978和1539nm激光所致上转换发光的增强作用

三价稀土离子上转换发光有着一些很有价值的应用技术:波导上转换及放大和激光、上转换三维立体显示、飞秒光谱应用、激光控温、三维成像与存储、光学温度感应系统、牙科等生物物理应用、上转换荧光防伪、上转换宽带光源、和上转换红外显示片等。因为受到太阳能电池发展需求的促进,上转换研究再度呈现出澎湃的研究热潮。目前,利用金属表面等离子体共振的近场增强效应能够有效增强其表面附近的荧光物质的发光的特性,有可能较大幅度的提高上转换发光的强度,从而有可能进一步把上转换发光推向实用。利用离子引入法,在铋化物的发光玻璃中引入银颗粒。研究结果表明银表面等离激元的表面等离子体共振吸收峰位于580～600 nm;而且,加热时间的延长导致了表面等离子体共振吸收峰的剧烈增强和稍微蓝移。978 nm半导体激光能够导致531.0, 546.0和657.5 nm的三组Er~(3+)的~2H_(11/2)→~4I_(15/2),~4S_(3/2)→~4I_(15/2),~4F_(9/2)→~4I_(15/2)的双光子上转换荧光, 978 nm激光激发掺铒铋化物发光玻璃的上转换发光的机理是第一步的~4I_(15/2)→~4I_(11/2)共振基态吸收和随后的第二步的~4I_(11/2)→~4F_(7/2)的共振激发态吸收;纳米银的表面等离激元的引入促成铋化物发光玻璃中铒离子的978 nm激光激发的上转换发光最大增强了272.0%倍。1 539 nm半导体激光能够导致波长为528.0, 547.0, 657.0和795.0 nm的四组Er~(3+)的~2H_(11/2)→~4I_(15/2),~4S_(3/2)→~4I_(15/2),~4F_(9/2)→~4I_(15/2)和~4I_(9/2)→~4I_(15/2)的上转换荧光; 1539 nm激光导致的528.0 nm ~2H_(11/2)→~4I_(15/2)和547.0 nm ~4S_(3/2)→~4I_(15/2)上转换荧光的机理主要是1 539 nm激光的~4I_(15/2)→~4I_(13/2),~4I_(13/2)→~4I_(9/2)和~4I_(9/2)→~2H_(11/2)的三步光激发吸收跃迁过程, 1 539 nm激光导致的657.0 nm ~4F_(9/2)→~4I_(15/2)上转换荧光的机理主要是1 539 nm激光的~4I_(15/2)→~4I_(13/2),~4I_(13/2)→~4I_(9/2)和~4I_(11/2)→~4F_(9/2)的三步光激发吸收跃迁过程;纳米银的表面等离激元的引入导致了铋化物发光玻璃中铒离子的1 539 nm激光激发的上转换发光最大增强160.3%倍。显然,靠近银表面等离激元共振吸收峰的978 nm激光上转换的增强效果比1 539 nm激光的要好。     

ErP5O14非晶中Er^3＋离子光谱参数的计数

由测量的ErP_5O_(14)非晶的吸收光谱,计算了Er~(3+)在五磷酸盐非晶中的强度参数Ω_λ,并由此计算了激光能级的振子强度、自发辐射跃迁速率、荧光分支比和积分发射截面。     

Effect of concentration quenching on the spectroscopic properties of Er~(3+)/Yb~(3+) co-doped AlF_3-based glasses

A series of highly Er~(3+)/Yb~(3+) co-doped fluoroaluminate glasses have been investigated in order to develop a microchip laser at 1.54 μm under 980 nm excitation. Measurements of absorption, emission and upconversion spectra have been performed to examine the effect of Er~(3+)/Yb~(3+) concentration quenching on spectroscopic properties. In the glasses with Er~(3+) concentrations below 10 mol%, concentration quenching is very low and the Er~(3+)/Yb~(3+) co-doped fluoroaluminate glasses have stronger fluorescence of 1.54μm due to the ~4I_(13/2)→~4I_(15/2) transition than that of Er~(3+) singly-doped glasses. As Er~(3+) concentrations above 10 mol% in the Er~(3+)/Yb~(3+) co-doped samples, concentration quenching of 1.54μm does obviously occur as a result of the back energy transfer from Er~(3+) to Yb~(3+). To obtain the highest emission efficiency at 1.54μm, the optimum doping-concentration ratio of Er~(3+)/Yb~(3+) was found to be approximately 1:1 in mol fraction when the Er~(3+) concentration is l     

Sm_xLa_(1-x)P_5O_(14)和Dy_xY_(1-x)P_5O_(14)晶体的荧光寿命研究

本文用脉冲衰减法和时间分辨荧光光谱法测量了六种不同稀土离子浓度的Sm_xLa_(1-x)P_5O_4晶体的~4G_(5/2)→~6H_J(J=5/2,7/2,9/2,11/2)四个能级和七种不同稀土离子浓度的Dy_xY_(1-x)P_5O_(14)晶体的~4F_(9/2)→~6H_J(J=15/2,13/2,11/2,9/2)四个能级的荧光寿命和荧光强度。结果指出,在这类晶体中,Sm~(3+)和Dy~(3+)的荧光寿命随着离子的浓度增加而变短,存在着严重的荧光浓度猝灭现象。最后还讨论了浓度与寿命,寿命与荧光强度的关系。     

Er~(3+)/Tm~(3+)共掺铋硅酸盐玻璃2.0μm光谱性质（英文）

用高温熔融法制备了Er~(3+)/Tm~(3+)共掺杂无铅铋硅酸盐玻璃.测试了玻璃的吸收光谱和荧光光谱,分析和表征了Er~(3+)、Tm~(3+)离子之间的能量传递机制和传递效率,结果表明:在800 nm和1 550 nm光源泵浦下,Er~(3+)的掺入能够增强Tm~(3+)离子1.8μm发光,相应的最大发射截面分别为6.7×10~(-21)cm~2和7.3×10~(-21)cm~2,荧光带宽达到250 nm.根据Dexter-Foster模型,得到Er~(3+):~4I_(13/2)能级到Tm~(3+):~3F_4能级的直接能量传递系数为16.8×10~(-40)cm~6/s,为1 550 nm泵浦下获得较强的1.8μm发光奠定了基础.     

K_5Bi_(0.9)Er_(0.1)(MoO_4)_4的晶体生长和光学性质

在化学计量的熔料里,用提拉法生长了K_5Bi_(0.9)Er_(0.1)(MoO_4)_4单晶。该晶体属于三方晶系,空间群为Rm,z=1.5,晶胞参数为a=6.029,c=20.823(六方表示)。晶体具有层状结构,沿着(0001)面容易解理。晶体在室温下的吸收光谱包括有若干条吸收带,它们是稀土离子所特有的。其中三个主要的吸收峰分别相当于从Er~(3+)离子的基态~4I_(15/2)向~4G_(11/2),~2H_(11/2)和~4I_(13/2)能级的跃迁。本文还给出晶体中相当于~4I_(13/2)→~4I_(15/2)跃迁的荧光发射光谱。     

Boson realization of YangiansY(sl(2)) andY(sl(3))

Studying the algebraic structure of the YangiansY(sl(2)), andY(sl(3)) we present their boson realizations. In the case ofY(sl(2)) we give the realization by using 1-canonical boson pair and two parameters and in theY(sl(3)) with 2-canonical boson pairs, two parameters and subalgebrasl(2). Substituting the realization ofU(sl(2)), we can obtain the pure boson realization by 3-canonical pairs and three parameters.Presented at the 4th Colloquium Quantum Groups and Integrable Systems, Prague, 22–24 June 1995.     

(Fe0.03Ni0.97)8(Si0.79P0.21)3的等温状态方程研究

 采用固态高温烧结反应方法,成功合成出了陨硅镍铁石样品(Fe_0.03Ni_0.97)₈(Si_0.79P_0.21)₃。X射线衍射结果表明,合成样品的结构为R3'c,对应的晶胞参数为a=b=0.663 8(1) nm,c=3.789 2(2) nm,V=1.446 15(6) nm³。在室温下,对样品进行原位高压X射线衍射研究,实验最高压力达到21.3 GPa,随着压力的升高,晶胞体积逐渐减小,但并没有观察到结构相变。利用Birch-Murnaghan状态方程对体积与压力的关系进行拟合,获得常温常压下的体积V₀=1.441 4(24) nm³,体积模量K₀=220(7) GPa。晶轴与压力的关系利用Murnaghan状态方程拟合,获得a轴和c轴的模量分别为K_a=257(9)和K_c=165(4),c轴较a轴容易压缩。     

Theoretical Study of the Collision-Induced Double Transition CO(2) (nu(3) = 1) + N(2) (nu(1) = 1) <-- CO(2) (nu(3) = 0) + N(2) (nu(1) = 0) at 296 K

A procedure is presented for the calculation of the double vibrational collision-induced absorption CO(2) (nu(3) = 1) + N(2) (nu(1) = 1) <-- CO(2) (nu(3) = 0) + N(2) (nu(1) = 0) on the basis of quantum lineshapes computed using an isotropic potential and dipole-induced dipole functions. The linestrengths and energies of the vibration-rotation transitions are treated explicitly for N(2), utilizing the HITRAN database for CO(2). The theoretical absorption profile is compared to recent experimental results. By narrowing the width of the individual lines contributing to the overall absorption profile relative to their values determined for N(2)-N(2) collision-induced absorption, excellent agreement between theory and experiment is obtained. Copyright 2000 Academic Press.     

Recording of second-harmonic index gratings in photorefractive (K(0.5) Na(0.5))(0.2) (Sr(0.75) Ba(0.25))(0.9) Nb(2)O(6) crystals

We propose and demonstrate a novel method for recording second-harmonic volume index gratings in photorefractive crystals. The fundamental component of the index grating is eliminated by means of a pi -phase shifted double-exposure process that uses the Mach-Zehnder interferometric technique. Experimental results for (K(0.5) Na(0.5)) (0.2)(Sr> (0.75)Ba (0.25))(0.9)Nb (2)O(6) crystals are presented and discussed.     

Measurement of G(E(p))/G(M(p)) in e(-->)p---> e(-->)p to Q(2) = 5.6 GeV(2)

The ratio of the electric and magnetic form factors of the proton G(E(p))/G(M(p)), which is an image of its charge and magnetization distributions, was measured at the Thomas Jefferson National Accelerator Facility (JLab) using the recoil polarization technique. The ratio of the form factors is directly proportional to the ratio of the transverse to longitudinal components of the polarization of the recoil proton in the elastic e(-->)p---> e(-->)p reaction. The new data presented span the range 3.5< Q(2)< 5.6 GeV(2) and are well described by a linear Q(2) fit. Also, the ratio sqrt[Q(2)] F(2(p))/F(1(p)) reaches a constant value above Q(2) = 2 GeV(2).     

Dual nature of the electronic structure of (La(2--x--y)Nd(y)Sr(x))CuO(4) and La(1.85)Sr(0.15)CuO(4).

High resolution angle-resolved photoemission measurements have been carried out on (La(1.4--x)-Nd(0.6)Sr(x))CuO(4), a model system with static one-dimensional (1D) charge ordering (stripe), and (La(1.85)-Sr(0.15))CuO(4), a high temperature superconductor (T(c) = 40 K) with possible dynamic stripes. In addition to the straight segments near ( pi,0) and ( 0,pi) antinodal regions, we have identified the existence of spectral weight along the [1,1] nodal direction in the electronic structure of both systems. This observation of nodal state, together with the straight segments near antinodal regions, reveals the dual nature of the electronic structure of stripes due to the competition of order and disorder.     

First Observation of the nu(17)-nu(4) Difference Bands of Diborane (10)B(2)H(6) and (11)B(2)H(6)

An analysis of the nu(17)-nu(4) difference bands near 800 cm(-1) of two isotopic species, (10)B(2)H(6) and (11)B(2)H(6), of diborane has been carried out using infrared spectra recorded with a resolution of ca. 0.003 cm(-1). In addition, the nu(17) band of (10)B(2)H(6) has been recorded and assigned. Since this band in (11)B(2)H(6) had already been studied (R. L. Sams, T. A. Blake, S. W. Sharpe, J.-M. Flaud, and W. J. Lafferty, J. Mol. Spectrosc. 191, 331-342 (1998)), it was possible to derive precise energy levels and Hamiltonian constants for the 4(1) vibrational states of both isotopic species. Copyright 2000 Academic Press.     

The v(1)+v(3) Bands of the (16)O(17)O(16)O and (16)O(16)O(17)O Isotopomers of Ozone

Using 0.002 cm(-1) resolution Fourier transform absorption spectra of an (17)O enriched ozone sample, an extensive analysis of the v(1)+v(3) bands of the (16)O(17)O(16)O and (16)O(16)O(17)O isotopomers of ozone has been performed for the first time. The experimental rotational levels of the (101) vibrational states were satisfactorily reproduced using a Hamiltonian matrix that takes into account the observed rovibrational resonances. More precisely, for (16)O(17)O(16)O, as for the other C(2v)-type ozone isotopomers, it was necessary to account for the Coriolis type resonances linking the (101) rotational levels with the levels of the (200) and (002) vibrational states and the Darling-Dennison interaction coupling the levels of (200) with those of (002). For the C(s)-type isotopomer, namely (16)O(16)O(17)O, as for (16)O(16)O(18)O and (16)O(18)O(18)O, it proved necessary to also account for an additional DeltaK(a)&equals+/-2 resonance involving the rotational levels from (101) and (002) (J.-M. Flaud and R. Bacis, Spectrochimica Acta Part A 54, 3-16 (1998)). Using a Hamiltonian matrix which takes these resonances explicitly into account, precise vibrational energies and rotational and coupling constants were deduced, leading to the following band centers: v(0)(v(1)+v(3))=2078.3496 cm(-1) for (16)O(17)O(16)O and v(0)(v(1)+v(3))=2098.8631 cm(-1) for (16)O(16)O(17)O. Copyright 2001 Academic Press.     

Theoretical Study of Collision-Induced Double Transitions in CO(2)-X(2) (X(2) = H(2), N(2), and O(2)) Pairs

The double vibrational collision-induced absorptions CO(2) (nu(3) = 1) + X(2) (nu(1) = 1) <-- CO(2) (nu(3) = 0) + X(2) (nu(1) = 0), for X(2) = H(2), N(2), and O(2) are studied on the basis of quantum lineshapes computed using isotropic potentials and dipole-induced dipole functions. The linestrengths and energies of the vibration-rotation transitions are treated explicitly for X(2) and utilizing the HITRAN database for CO(2). From the frequency-dependent absorption profiles, the integrated absorption intensities are determined to be 7.2 +/- 1.2, 1.2 +/- 0.1, and 1.1 +/- 0.2 (10(-4) cm(-2) amagat(-2)) for the H(2), N(2), and O(2) collision partners, respectively. The integrated intensities for H(2) and N(2) agree well with previously measured and calculated results, while the value for O(2), which represents the first theoretical determination for this absorption, is approximately four times greater than the only experimental measurement (0.29 x 10(-4) cm(-2) amagat(-2)). Copyright 2001 Academic Press.