NO2 在第二电子吸收带的光解

运用单光子激光诱导荧光方法,研究了NO2分子在第二吸收带的光解反应动力学.首次报道了NO2(B2B2态)光解初生态产物NO自由基的v″=1,2的转动分布.发现了NO自由基v″=1的明显双模式分布.进而提出了可能有两种竞争机理控制该反应.     

乙烯自由基~2A″(v′=0)←~2A′(v″=0)带的转动分析

通过193nm光解丁烯酮分子产生乙烯基自由基(·C2H3).经射流冷却后,用另一束激光光解·C2H3,生成的氢原子碎片经共振增强多光子电离(REMPI)过程,记录氢离子信号随光解波长变化,得到20020～20070cm-1范围内乙烯基激发的转动分辨光谱.该谱对应于A$2A″(v′=0)%X$2A′(v″=0)跃迁的转动结构.结合量子化学理论计算、光谱拟合以及前人的研究结果,对该段光谱进行了完整的转动识别,确定了40条转动谱线的位置.由光谱拟合还得到A$2A″(v′=0)能级的预解离寿命为3.3ps,且不依赖于转动量子数.     

乙烯自由基(A)2A″(v′=0)←(X)2A′(v"=0)带的转动分析

通过193 nm光解丁烯酮分子产生乙烯基自由基(·C2H3).经射流冷却后,用另一束激光光解·CaH3,生成的氢原子碎片经共振增强多光子电离(REMPI)过程,记录氢离子信号随光解波长变化,得到20020～20070 cm-1范围内乙烯基激发的转动分辨光谱.该谱对应于(A)2A″(v′=0)←(X)aA′(v″=0)跃迁的转动结构.结合量子化学理论计算、光谱拟合以及前人的研究结果,对该段光谱进行了完整的转动识别,确定了40条转动谱线的位置.由光谱拟合还得到(A)2A″(v′=0)能级的预解离寿命为3.3 ps,且不依赖于转动量子数.     

氦液滴中羰基硫分子的光解动力学

用时间切片速度成像方法研究了氦液滴中羰基硫(COS)分子的光解动力学. 从共振增强(2+1)电离的CO光谱中发现在氦液滴环境中解离产物CO的转动冷却比振动冷却更有效.利用速度成像采集到的CO (v=0)和CO (v=1)的影像在角分布上都呈现出各向同性的特点. 产物平动能分布的结果表明尽管大部分的平动能都被超流体环境所弛豫, 但振动激发态产物CO (v=1) 的平均平动能比振动基态产物CO (v=0) 的平均平动能高.对羰基硫分子在氦液滴中的光解动力学机理进行了讨论.     

氧硫化碳在230 nm光激发下的S(~3P)解离通道

在230nm激光激发下,氧硫化碳(OCS)分子迅速解离生成振动基态但高转动激发的CO(X~1∑_g~+,v=0,J=42-69)碎片,并通过共振增强多光子电离技术实现其离子化。通过检测处于J=56-69转动激发态CO碎片的离子速度聚焦影像,我们获得了各转动态CO碎片的速度分布和空间角度分布,其中包含了S(1D)+CO的单重态和S(~3P_J)+CO三重态解离通道的贡献。不同的转动态CO碎片对应三重态产物通道的量子产率略有不同,经加权平均我们得到230 nm附近光解OCS分子中S(3P)解离通道的量子产率为4.16%。结合高精度量化计算的OCS分子势能面和吸收截面的信息,我们获得了OCS光解的三重态解离机理,即基态OCS(X~1A')分子吸收一个光子激发到弯曲的A~1A'态之后,通过内转换跃迁回弯曲构型的基电子态,随后在C-S键断裂过程中与2~3A"(c~3A")态强烈耦合并沿后者势能面绝热解离。     

CS21B2(1Σ+u)态预离解产物CS的振转布居研究

用一束波长为210.27 nm的激光将CS2分子激发至预离解态1 B2(1 Σ+u),用另一束激光通过激光诱导荧光(LIF)方法检测碎片CS,在250.5～286.5 nm获得了CS碎片A1 Π←X1 Σ+振转分辨的激发谱.通过对光谱强度的分析,获得了CS碎片v″=0～8的振动布居和v″=1,4～8振动态的转动布居.结果发现,碎片CS的振动布居呈双模结构,分别对应于CS2分子1 B2(1 Σ+u)态的两个解离通道,即CS(X1 Σ+,v″=0～9)+S(3PJ)和CS(X1 Σ+, v″=0～1)+S(1 B2).由此得到两个解离通道的分支比S(3PJ): S(1 B2)为5.6±1.2.与前人193 nm处的研究结果相比, 210.27 nm激发更有利于S(3PJ)通道的生成.此外,实验还发现CS的转动布居不满足热平衡分布,为两个Boltzmann分布的合成.     

Pu（^7Fg）＋H2（X^1∑g^＋,0,0）的分子反应动力学

基于PuH_2分子基态(X~7A_1)的分析势能函数，用准经典的Monte-Carlo轨线法 对Pu(~7Fg)+H_2(X~1∑_g~+，0，0)的分子反应动力学过程进行了计算。结果表明 ：Pu(~7F_g)与H_2(X~1∑_g~+，0，0)碰撞是弹性碰撞。     

排斥作用对光分解产物转动分布的重要性

本文用一个简单的经典力学模型, 对ClCN, BrCN, C_2N_2, C_4N_2等一系列分子的光分解产物的转动分布进行了分析, 着重讨论了光解碎片间的相互排斥对它们的转动分布的作用。模型分析和实验结果的比较表明, 这种经典模型对于理解光解过程的动力学行为是很有用的。     

单光子LIF方法研究亚硝基苯266 nm光解动力学

用266 nm激光解离亚硝基苯（C6H5NO) 产生光解碎片NO,并利用单光子激光诱导荧光(LIF)技术（X2Πν″=0→A2Σ+ν′=0）测得初生态光解产物NO的振转光谱。根据计算所得的模拟光谱对光解碎片NO（X,ν″＝0)的转动量子数J″进行了归属,得到量子数最大到J″＝50.5的各转动能级的相对布居,这表明光解碎片NO具有较高的转动激发。提出了C6H5NO在266 nm下可能的光解机理。     

激光诱导荧光法研究CN(V″=0,1)自由基与碳氢化合物的反应速率和机理

CN自由基与碳氢化合物的反应对于了解碳氢火焰中NO_x的形成、星球大气中氮的平衡具有重要的意义。以前主要是用宽带闪光光解含氰化合物,产生CN自由基,利用吸收方法临视CN基的浓度随时间的变化来测量反应速率。由于吸收方法灵敏度低,单色仪分辨率不高,难于准确获得不同振动能量CN基的反应速率。我们采用小功率的ArF193毫微米脉冲檄光器,每个光脉冲可产生CN基的数密度为～10~(12)分子厘米~(-3)。因此自由基间的反应可完全忽略。实验中选用C_2N_2作为光解物,光解产物为CN(V″=0,1)。跟踪V″=0,1的浓度随时间的变化,就可获得不同振动能量CN基的反应速率,从而了解振动能量对反应的影响。     

激光诱导荧光法研究CN(V″=0,1)自由基与碳氢化合物的反应速率和机理

The rate constants of eleven hydrocarbons and fluorocarbons with CN (V″=0, 1) at 300 K have been measured by using Laser Induced Fluorescence(LIF) method For the saturated hydrocarbons, the rate constants are changed from (5.6±0.3)×10~(-13) for CH_4 to (2.3±0.2)×10~(-10)cm~3 molecu~(-1).s~(-1) for C_7H_(16). The rate constants of the reaction of CN with alkenes and alkynes are close to the gas kinetic rate in spite of the structure of the molecules.The rate constants and mechanism of CN with the saturated hydrocarbons, H_2 and CH_3OH can be explained satisfactorily by the long distance attractive potential. The reaction of CN with alkenes and alkynes can only proceed through the addition into π bond. The influence of vibrational energy on the reaction rate was not found in the reactions of CN radical with hydrocarbon compounds.     

Vibrationally selective radiative and non-radiative transitions in gaseous hydrogen molecules

An efficient vibrationally selective technique to build-up the v″=1 vibrational levels in gaseous hydrogen is demonstrated using stimulated Raman pumping (SRP). Both photo-acoustic Raman spectroscopy (PARS) and coherent anti-Stokes Raman spectroscopy (CARS) are used to study non-radiative and radiative (v″=0 and v″=1) transitions in gaseous H(2) molecules. The population fraction in the v″=1 vibrational level has been estimated using combined photo-acoustic and coherent anti-Stokes Raman spectroscopy with stimulated Raman pumping.     

Rotational excitation and the energy distribution of CN(B2Σ) produced by the reaction of metastable Ar(3P0,2) atoms with HCN

The violet emission spectrum (B²ΣX²Σ) of the CN radical observed by the collision of HCN with metastable Ar(³P_0,2) atoms was analyzed. The effective rotational temperature of the CN(B²Σ) radical, as estimated from a band envelope analysis, is about 2000°K. The distributions of the excess energy to vibration, rotation and translation are found to be 1.2 ± 0.2, 0.2 and 1.9 ± 0.3 eV, respectively.     

Photoluminescence spectroscopy of the CN radical produced in the infrared photolysis of CH3CN

The infrared laser-induced photolysis of CH₃CN has been studied by observing luminescence from the excited CN (B²Σ⁺) radical and pulsed dye laser-induced fluorescence of ground state CN(X²Σ⁺), both produced as primary fragments. Both temporal and wavelength resolved spectroscopy have been performed on the luminescence, whereas pulsed dye laser probing has allowed time-resolution of the CN(X²Σ⁺) radical as well as measurements of the decay time of the CN(B²Σ⁺) state produced in the dye laser pumping. A reaction mechanism, characterizing the observed results, is proposed.     

Photodissociation of BrCN and ICN in the a continuum: Vibrational and rotational distributions of CN(X 2Σ+)

We report results of experiments on photodissociation of ICN and BrCN in the long-wavelength (A) continuum in which primary rotational and vibrational distributions of CN in its electronic ground state are determined. For the CN fragment from ICN, our observations at 222 and 249 nm, reported here, together with our earlier results at longer wavelengths, show that the fraction of energy which goes into rotation (in the ground-state channel) is very nearly independent of exciting wavelength in the range 222–351 nm. This holds for each of CN vibrational levels 0, 1, and 2, where the fractions are 15, 25, and 33% respectively. The vibrational distributions decrease monotonously with υ, but show little change as a function of exciting wavelength. CN distributions are also presented for the photodissociation of BrCN at 193, 222, 249, and 308 nm. Results for both parent molecules are briefly discussed in relation to other recent experimental and theoretical work.     

The microwave and millimeter rotational spectra of the PCN radical (X3Σ-)

The pure rotational spectrum of the PCN radical (X(3)Σ(-)) has been measured for the first time using a combination of millimeter/submillimeter direct absorption and Fourier transform microwave (FTMW) spectroscopy. In the millimeter instrument, PCN was created by the reaction of phosphorus vapor and cyanogen in the presence of an ac discharge. A pulsed dc discharge of a dilute mixture of PCl(3) vapor and cyanogen in argon was the synthetic method employed in the FTMW machine. Twenty-seven rotational transitions of PCN and six of P(13)CN in the ground vibrational state were recorded from 19 to 415 GHz, all which exhibited fine structure arising from the two unpaired electrons in this radical. Phosphorus and nitrogen hyperfine splittings were also resolved in the FTMW data. Rotational satellite lines from excited vibrational states with v(2) = 1-3 and v(1) = 1 were additionally measured in the submillimeter range. The data were analyzed with a Hund's case (b) effective Hamiltonian and rotational, fine structure, and hyperfine constants were determined. From the rotational parameters of both carbon isotopologues, the geometry of PCN was established to be linear, with a P-C single bond and a C-N triple bond, structurally comparable to other non-metal main group heteroatom cyanides. Analysis of the hyperfine constants suggests that the two unpaired electrons reside almost exclusively on the phosphorus atom in a π(2) configuration, with little interaction with the nitrogen nucleus. The fine structure splittings in the vibrational satellite lines differ significantly from the pattern of the ground state, with the effect most noticeable with increasing v(2) quantum number. These deviations likely result from spin-orbit vibronic perturbations from a nearby (1)Σ(+) state, suggested by the data to lie ~12,000 cm(-1) above the ground state.     

Dynamics of formation of CN(B2Σ+) fragment from HCN and DCN in an argon afterglow

The dissociative excitation of HCN and DCN producing CN(B²Σ⁺) in collision with Ar(³P_0,2) was investigated in a flowing afterglow. The Δν = 0, ?1, and ?2 sequences of the CN(BX) violet emission were analyzed by computer simulation, and the vibrational and rotational distributions of the CN(B²Σ⁺) fragment were obtained. Possible reaction pathways were studied on the basis of a linear surprisal analysis of the observed distributions and their isotope effects.     

The reaction products of the 193 nm photolysis of vinyl bromide and vinyl chloride studied by time-resolved Fourier transform infrared emission spectroscopy

Time-resolved Fourier transform infrared (TRFTIR) emission spectroscopy has been used to study the 193 nm photolysis of vinyl bromide (C(2)H(3)Br) and vinyl chloride (C(2)H(3)Cl). Time-resolved IR emission was analysed to obtain nascent vibrational state populations of two primary photolysis products: HBr (v = 1-7) and HCl (v = 1-6). In both cases the nascent vibrational state populations monotonically decrease with increasing v and are in excellent agreement with previously published data. Time-resolved populations were analysed to yield rate constants for vibrational relaxation of HBr (v = 1-3) and HCl (v = 1-4) by parent vinyl bromide and vinyl chloride, respectively. In both cases the rate constants were found to increase with increasing vibrational quantum number, in agreement with a single quantum de-excitation via vibrational to vibrational energy transfer. Butadiene (C(4)H(6)) was identified as a secondary product of the photolysis of both vinyl halides, and shown to be formed from the reaction of parent vinyl halide with the vinyl radical. The presence of a buffer gas was found to produce a strong emission feature centred at 2,200 cm(-1), the intensity of which was dependent on the pressure of the buffer gas used, and whose kinetics are indicative of a secondary reaction product. We propose that this emission is from the vibrational progression of the electronic transition A(0, v, 1) --> X(0, v, 2) in the secondary reaction product C(2)H, whose formation route is favoured by the presence of buffer gas.