超高泵浦功率下的Xe(6p[1/2]_0,6p[3/2]_2和6p[5/2]_2)原子的能量转移过程（英文）

本文研究了Xe(6p[1/2]_0,6p[3/2]_2和6p[5/2]_2)原子在聚焦条件下的动力学过程.激发能级的原子密度在聚焦条件下会显著地增加,因此两个高激发态原子之间的energy-pooling碰撞的概率也会增加.这种energy-pooling碰撞主要有三种类型.第一种类型为energy-pooling碰撞导致的电离,一旦将激发激光聚焦,就可以从侧面的窗口观察到非常明显的电离现象,不论激发能级是6p[1/2]_0、6p[3/2]_2或6p[5/2]2能级.这种电离的产生机理是energy-pooling电离或者一个Xe*原子再吸收一个光子产生电离.第二种类型为跨越较大能极差的energy-pooling碰撞.当激发能级为6p[1/2]_0能级的情况下,两个6p[1/2]_0原子碰撞会产生一个5d[3/2]_1原子和一个6s'[1/2]_0原子.第三种类型为跨越较小能级差的energy-pooling碰撞.以5个二次产生的6p能级为上能级的荧光强度都变得更强,并且这些荧光的上升沿都变得更陡峭.产生这些6p原子的主要机理是energy-pooling碰撞并非简单的碰撞弛豫.基于理想气体原子之间的碰撞概率公式,推导出两个6p[1/2]。原子的energypooling碰撞速率为6.39×10~8 s~(-1).此外,6s原子在聚焦条件下的密度也会增加.因此所有的荧光曲线会因为辐射俘获效应而出现非常严重的拖尾.     

XeO^＊和Xes^＊紫外荧光的某些特性

研究了在Xe(6p)激发态与N_2O和OCS反应中,产物XeO~*和XeS~*的紫外荧光特性.实验证实它们具有短的寿命以及发射谱在高压Ar中的振动弛豫效应.     

Resonance-Enhanced Photon Excitation Spectroscopy of the Even-Parity Autoionizing Rydberg States of Xe

用脉冲直流放电产生Xe原子亚稳态5p56s[3/2]2和5p56s′[1/2]0.在单光子28000－42000cm-1能量范围内,结合飞行时间质谱技术获得Xe原子共振增强激发光谱.光谱分析表明,所有谱线来源于Xe原子5p56s[3/2]2和5p56s′[1/2]0两个亚稳态吸收单个光子向偶宇称np′、nf′自电离Rydberg态序列的跃迁.实验观测到许多新的自电离能级,并获得更精确和系统的能级位置和量子亏损值数据.     

F2 Σ+ -X 2Σ +Band System of Cobalt Carbide

用脉冲直流放电产生Xe原子亚稳态5p56s[3/2]2和5p56s′[1/2]0.在单光子28000－42000cm-1能量范围内,结合飞行时间质谱技术获得Xe原子共振增强激发光谱.光谱分析表明,所有谱线来源于Xe原子5p56s[3/2]2和5p56s′[1/2]0两个亚稳态吸收单个光子向偶宇称np′、nf′自电离Rydberg态序列的跃迁.实验观测到许多新的自电离能级,并获得更精确和系统的能级位置和量子亏损值数据.     

低气压下XeCl准分子的形成研究

本工作利用高频介质阻挡放电对较低气压(70～1330 Pa)Xe/Cl_2混合气体中XeCl准分子的形成过程进行研究。通过探测不同Xe/Cl_2混合气压和不同Xe/Cl_2混合比条件下放电等离子体在285～315nm波长范围的荧光发射谱,得到了XeCl准分子在308nm附近的荧光发射以及荧光强度随气压变化曲线。得出该实验条件下生成XeCl准分子的最佳Xe/Cl_2混合比为4:1。     

多价抗衡离子诱导聚甲基丙烯酸N,N-二甲基氨基乙酯(PDMAEMA)刷构象转变的UCST行为

本文应用分子场理论,研究pH、[Fe(CN)_6]~(3-)诱导聚甲基丙烯酸N,N-二甲基氨基乙酯(PDMAEMA)刷的上临界溶解温度(UCST)构象转变与结构特性.理论模型考虑p H和[Fe(CN)_6]~(3-)对PDMAEMA刷体系的静电调控作用.研究发现,在不同[Fe(CN)_6]~(3-)浓度、不同p H条件下,PDMAEMA刷呈现了UCST构象转变行为.由于p H调节PDMAEMA单体质子化,[Fe(CN)_6]~(3-)通过与PDMAEMA带正电荷的单体结合,形成了在PDMAEMA链内以[Fe(CN)_6]~(3-)为中介的带电单体间的静电吸引结合.随着温度升高,[Fe(CN)_6]~(3-)与PDMAEMA带正电荷的单体结合被破坏,[Fe(CN)_6]~(3-)在链内凝聚导致的静电屏蔽效应减弱,PDMAEMA链内带电单体间的静电排斥增强,PDMAEMA刷的构象呈现了从塌缩到溶胀的UCST转变行为,并且在较高[Fe(CN)_6]~(3-)浓度条件下,PDMAEMA刷构象转变的UCST增高.在较低p H值条件下,较多的PDMAEMA单体被质子化,[Fe(CN)_6]~(3-)与PDMAEMA带正电单体的结合增强,PDMAEMA刷构象转变的UCST增大.基于pH和[Fe(CN)_6]~(3-)对PDMAEMA刷体系中的静电调控效应,可以预言,在较小p H和较大[Fe(CN)_6]~(3-)浓度条件下,PDMAEMA链在垂直培基表面沿着链方向形成结节状结构.这是由于以[Fe(CN)_6]~(3-)为中介的链内带电单体间的静电吸引作用增强,导致临近单体间汇聚结节.我们的理论结果符合实验观测,由此表明,pH调节PDMAEMA单体的带电状态,以及[Fe(CN)_6]~(3-)在PDMAEMA链内凝聚导致的静电屏蔽效应,决定着PDMAEMA刷的UCST构象转变和结构特性.     

Ca(BH_4)_2络合物电子结构及热力学稳定性的第一性原理研究

利用第一性原理研究了低温及高温相Ca(BH_4)_2络合物的电子结构、晶格振动及其反应焓.计算结果表明:低温及高温相Ca(BH_4)_2中Ca~(+2)与[BH_4]~-以离子键形式相结合,[BH_4]~-离子中B原子和H原子以共价键形式相结合,对该共价键有贡献的主要是B原子的2p轨道电子,H原子的1s轨道电子.Ca(BH_4)_2可能的反应路径为:Ca(BH_4)_2→2CaH_2+CaB_6+10H_2,该反应在300 K下反应焓为43.22 kJ/molH_2.拉伸B—H键所对应的声子频率较高,其值为2360～2500 cm~(-1),这可能是导致B—H键断裂释放氢气需要较高温度的主要原因之一.     

亮菌甲素荧光熄灭法测定微量铁

基于铁对亮菌甲素的荧光熄灭 ,建立了测定微量铁 ( )的新方法。在 p H8.81的硼砂缓冲体系中 ,最大激发波长和发射波长分别为 2 81nm和 4 6 2 nm,亮菌甲素的荧光强度与铁 ( )的加入量在 0 .0 0 5—0 .4 5 0 μg/ m L间存在线性关系 ,检出限为 0 .6 μg/ L Fe( )。方法操作简便、反应迅速、灵敏度高、选择性好 ,用于环境水样中痕量 Fe( )的测定 ,结果令人满意     

圆偏振飞秒激光脉冲与低压氙气体靶相互作用软X射线辐射实验研究

利用平场光栅谱仪,分别在2和3 kPa的低气压下,测量了脉宽35 fs的圆偏振超强超短激光脉冲与5 mm长氙气体靶相互作用产生的波长在5～60 nm范围内的离子谱线。2 kPa时最强的跃迁为XeⅧ：4d105s(2S_1/2)—4d95s5p(2P_3/2)的17.085 6 nm线,3 kPa时最强的跃迁为11.343 nm的XeⅦ 4d105s2(1S0)—4d95s25f(3P₁)跃迁。两种气压下,Xe均被电离到XeⅦ,XeⅧ,XeⅨ态。     

[Na(15-C-5)]2[Pd(SCN)4]配合物的合成与结构分析

研究了15-冠-5(15-C-5)与Na2[Pd(SCN)4]的反应,得到的配合物[Na(15-C-5)]2[Pd(SCN)4]通过元素分析、红外光谱、单晶X射线衍射进行了结构分析.该配合物为单斜晶系,空间群C2/c,晶体学数据: a=1.3525(6)nm,b=1.3729(6)nm,c=2.0312(9)nm,β=102.985(6)°,V=3.675(3)nm3,Z=4,F(000)=1696,R1=0.0288,wR2=0.0457.结构分析表明,该配合物由两个[Na(15-C-5)]+配阳离子和一个[Pd(SCN)4]2-配阴离子组成,二者通过Na-N相互作用形成二维网状结构.     

超高泵浦功率下的Xe(6p[1/2]0, 6p[3/2]2, 和6p[5/2]2)原子的能量转移过程

本文研究了Xe(6p[1/2]₀, 6p[3/2]₂, and 6p[5/2]₂)原子在聚焦条件下的动力学过程. 激发能级的原子密度在聚焦条件下会显著地增加,因此两个高激发态原子之间的energy-pooling碰撞的概率也会增加. 这种energy-pooling碰撞主要有三种类型. 第一种类型为energy-pooling碰撞导致的电离. 一旦将激发激光聚焦,就可以从侧面的窗口观察到非常明显的电离现象,不论激发能级是6p[1/2]₀、6p[3/2]₂或6p[5/2]₂能级. 这种电离的产生机理是energy-pooling电离或者一个Xe^*原子再吸收一个光子产生电离. 第二种类型为跨越较大能极差的energy-pooling碰撞. 当激发能级为6p[1/2]₀能级的情况下,两个6p[1/2]₀原子碰撞会产生一个5d[3/2]₁原子和一个6s''[1/2]₀原子. 第三种类型为跨越较小能级差的energy-pooling碰撞. 以5个二次产生的6p能级为上能级的荧光强度都变得更强,并且这些荧光的上升沿都变得更陡峭. 产生这些6p原子的主要机理是energy-pooling碰撞并非简单的碰撞弛豫. 基于理想气体原子之间的碰撞概率公式,推导出两个6p[1/2]₀原子的energy-pooling碰撞速率为6.39x10⁸s^-1. 此外,6s原子在聚焦条件下的密度也会增加. 因此所有的荧光曲线会因为辐射俘获效应而出现非常严重的拖尾.     

N_2(B~3Ⅱ_g)高振动态在Xe原子中的碰撞激发和弛豫

在用双光子激发产生的Xe(5p~56p)原子与N_2分子碰撞过程中,有效地生成了N_2(B~3П_g,v=9～14)振动激发态.观察到相应的Δv=4的N_2(B~3П_g-A~3∑_u~+)辐射跃迁萤光,测量了Xe(6p)原子在N_2中的淬灭速率常数,对碰撞弛豫过程进行了讨论.     

Experimental verification of a zero-dimensional model of the kinetics of XeCl* discharges by XeCl*(B)-, XeCl*(C)-, and Xe2Cl*-density measurements

Absolutely calibrated emission spectroscopy has been used to determine the particle number densities of XeCl^*(B), XeCl^*(C), and Xe₂Cl^* in a small scale Ne/Xe/HCl discharge with well-defined current and voltage pulses for a wide range of parameters. The measured particle number densities could be reproduced quite well by numerical model calculations using the rate-coefficient values of Quiñones et al. [1] for the quenching of XeCl^*(B,C) by Ne, Xe, and 2Xe, but 3.0 × 10^–31 cm⁶/s for the formation of Xe₂Cl^* by (Ne + Xe)-quenching. For the electron quenching, we recommend a rate coefficient value of 3.2 × 10^–8 cm³/s. From the equilibrium ratio of the particle number densities of XeCl^*(C) and XeCl^*(B), the energy separation between these states has been estimated to be 72 ± 33 cm^–1 with the B state placed above the C state.     

Circular polarization of ion fluorescence completing the analysis of resonant Xe* 4d(-1)(5/2)6p Auger decay

The relative contributions of the partial electron waves emitted in the Auger decay of the Xe* 4d(-1)(5/2)6p(J(*)=1) resonance have been determined by fluorescence polarimetry after excitation with circularly polarized synchrotron radiation. The analysis of circularly polarized fluorescence of the photoion leads to an independent determination of the orientation parameters for all states of the Xe II 5p(4)6p multiplet. The present study provides, in combination with data on the angular distribution and spin polarization of the Auger electrons, complete quantum mechanical information on the resonant Auger decay, i.e., branching ratios and relative phases of the Auger decay amplitudes.     

Multiphoton mass spectra of XeKr molecules in the range of excited Xe*6<Emphasis Type="Italic">p</Emphasis>[5/2]<Subscript>2, 3</Subscript> atoms

Data on excited states of XeKr molecules in the energy range 78280–77600 cm^?1 are obtained. Using the method of multiphoton laser photoionization of molecules in a supersonic jet, five vibrational progressions of XeKr molecules are obtained, which are attributed to five electronic-vibrational transitions from the ground state of the XeKr molecule of the symmetry 0⁺ to excited states of the symmetry Ω = 0⁺, 1, 2 with the dissociation limit Kr¹ S ₀ + Xe*6p[5/2]₂ and of the symmetry Ω = 1, 2 with the dissociation limit Kr + Xe*6 p [5/2]₃. The molecular constants of the corresponding excited states of the XeKr molecule are estimated.     

低速Xe~(q+)(4≤q≤20)离子与Ni表面碰撞中的光辐射

实验中测量了0.38V_(Bohr)(460 keV)高电荷态Xe~(q+)(4≤q≤20)离子轰击高纯Ni表面发射的400-510 nm光谱.实验结果包括NiⅠ原子谱线,NiⅡ离子谱线,以及入射离子中性化发射的XeⅠ,XeⅡ和XeⅢ谱线.研究了谱线XeⅡ410.419,XeⅢ430.444,XeⅡ434.200,XeⅡ486.254,NiⅠ498.245,NiⅠ501.697,NiⅠ503.502,NiⅠ505.061和NiⅠ508.293 nm的光子产额随着入射离子电荷态的变化.结果表明,入射离子中性化和溅射Ni原子发射谱线的光子产额随着入射离子电荷态的增加而增加,其趋势与入射离子势能一致.     

UV Radiation of Low Pressure XeCl* and KrCl* Glow Discharges

The positive column of low pressure DC glow discharges in Xe/Cl₂ and Kr/Cl₂ gas mixtures has been investigated with respect to its UV radiation power and radiative efficiency for a wide range of parameters (total gas pressure: 1–30 mbar, current 10–30 mA, partial pressure of Cl₂: 1–33%). Also the radial distribution of the particle number densities of XeCl* (B) and KrCl* (B) has been determined by absolutely calibrated emission spectroscopy. Optimum UV (190–350 nm) output and efficiency has been found in gas mixtures with a relative Cl₂ partial pressure of 2–3% and total gas pressure of 12–18 mbar. At these parameters, the UV radiation power per column length is greater than 40 Watt/m with a radiative efficiency of 15–18%. These discharges could be used for UV induced photochemical processes.     

Discovery of dumbbell-shaped Cs*Hen exciplexes in solid 4He

We have observed several new spectral features in the fluorescence of cesium atoms implanted in the hcp phase of solid helium following laser excitation to the 62P states. Based on calculations of the emission spectra using semiempirical Cs-He pair potentials the newly discovered lines can be assigned to the decay of specific Cs*Hen exciplexes: an apple-shaped Cs(APi3/2)He2 and a dumbbell-shaped Cs(APi1/2)Hen exciplex with a well-defined number n of bound helium atoms. While the former has been observed in other environments, it was commonly believed that exciplexes with n>2 might not exist. The calculations suggest Cs(APi1/2)He7 to be the most probable candidate for that exciplex, in which the helium atoms are arranged on a ring around the waist of the dumbbell-shaped electronic density distribution of the cesium atom.     

On the correlation between the composition of Pr doped garnet type materials and their photoluminescence properties

Lu₃(Al,Ga)₅O₁₂ and (Y,Lu)₃(Al,Mg,Si)₅O₁₂ samples doped with 1% Pr³⁺ were prepared by two aqueous sol-gel chemistry approaches, such as citrate and glycolate methods. All samples were characterised by powder X-ray diffraction (XRD), thermal quenching (TQ), fluorescence lifetime measurements and photoluminescence (PL) techniques. It turned out that the Pr³⁺ emission is very sensitive to the composition of the garnet host lattice. Lu₃Al₅O₁₂:Pr³⁺ samples showed mainly [Xe]4f¹5d¹→[Xe]4f² broad band emission in UV-blue region, whereas [Xe]4f²-[Xe]4f² line emission of Pr³⁺ dominated in Lu₃Ga₅O₁₂ samples. Modification of garnet crystals with Mg²⁺-Si⁴⁺ pair has led to generation of strong crystal field strength resulting in energy transfer from 5d to 4f orbitals. Y₃AlMg₂Si₂O₁₂ composition generated the strongest crystal field splitting out of all synthesised samples and showed practically only Pr³⁺ [Xe]4f²-[Xe]4f² line emission in the red spectral region.