VO分子2△3/2—12△3/2电子跃迁P线系发射谱线的研究

本文利用孙卫国课题组建立的能精确计算(预言)某双原子分子电子态P线系发射谱线的物理新公式,首次研究了VO分子从电子态~2△3/2跃迁到电子态1~2△3/2的(0,0)跃迁带中的P线系发射谱线.获得的研究结果不仅重复了实验上己知的低转动态谱线数据,而且还正确预言了该跃迁带在实验上难以精确测量的转动量子数J=80.5以内的高振转激发态的P线系发射光谱.为研究VO分子内部结构提供了重要的物理信息.     

VO分子2^Δ3/2-1^2Δ3/2电子跃迁P线系发射谱线的研究

本文利用孙卫国课题组建立的能精确计算（预言）某双原子分子电子态P线系发射谱线的物理新公式, 首次研究了VO分子从电子态^2Δ3/2跃迁到电子态1^2Δ3/2的（0, 0）跃迁带中的P线系发射谱线. 获得的研究结果不仅重复了实验上已知的低转动态谱线数据,而且还正确预言了该跃迁带在 实验上难以精确测量的转动量子数J=80.5以内的高振转激发态的P线系发射光谱. 为研究VO分子内部结构提供了重要的物理信息.     

精确研究NbN分子d1Σ+—b1Σ+电子态跃迁的P线系发射光谱

本文利用最近建立的能精确求解双原子分子P线系发射光谱的物理新公式, 研究了NbN分子从电子态d¹Σ⁺向b¹Σ⁺电子态跃迁中(1,1)跃迁带的P支发射光谱. 获得的计算结果不仅很好地重现了已知低转动态的实验谱线数据, 同时也预言了该跃迁带包含转动量子数J=80在内的高振转激发态的精确P线系发射光谱. 该方法在理论上为实验技术难以精确测量的双原子分子体系提供了一种获得精确的高激发态谱线数据的物理新方法. 从而可以为那些需要NbN分子高激发态跃迁谱线的研究工作提供必要的数据.     

Cl2+离子R支跃迁光谱的理论研究

从双原子分子能级的物理表达式出发进行多次微分,建立了预测双原子分子体系R支高振转跃迁谱线的新解析公式. 使用新解析公式预测双原子体系R支高阶跃迁谱线的数据时,最多只需15条精确的实验跃迁谱线和该跃迁带中对应的上下 振动态的转动光谱常数B′_v 和 B″_v.将该解析公式用于预测Cl₂⁺ 离子 A²∏_u---X²∏_g跃迁系(3,7)带和(4,8)带的跃迁谱线,不仅精确的重复了实验给出的较低阶的跃迁光谱数据值, 而且正确预言了所研究体系中缺失的振转跃迁谱线,尤其是高阶的跃迁谱线数据.     

NO分子b4Σ--a4Πi(4,0)带的吸收光谱

通过对NO与He流动混合气体放电, 产生了激发态的NO(a⁴Π_ii) 分子. 利用光外差-浓度调制吸收光谱技术测量了NO分子在12530-12850 cm^-1波段内的吸收光谱, 并标识出b⁴Σ^--a⁴Π_i(4,0)带在该波段内的324条光谱跃迁谱线. 采用标准⁴Σ^--⁴Π_i哈密顿量模型, 通过非线性最小二乘法拟合其中267条谱线, 拟合残差(0.0071 cm^-1) 接近实验系统测量误差(0.007 cm^-1). 获得的主要分子常数与文献提供的常数符合, 并且拟合得到了精细结构分子常数.     

N2第二正带系发射光谱的理论计算及实验研究

本文利用分子光谱理论系统的计算和分析N₂第二正带系(C³∏_u→B³∏_g)的发射光谱, 以研究光谱强度的分布规律与不同温度条件和气体条件的关系. 基于N₂的三重态能级结构特性, 重点计算和讨论了发射光谱的概个重要参数: 通过求解高、低电子态的哈密顿矩阵得到了振转能级特性; 利用r质心近似法求取了能级间跃迁的电偶极矩函数和爱因斯坦跃迁概率; 进而计算了不同振动和转动温度条件下谱线的强度分布. 进行了N₂和Ar的混合放电实验, 利用实验光谱数据同理论结果进行拟合分析, 确定了N₂分子的振动温度和转动温度分别约为4300 K和800 K. 另外由于潘宁离化效应, N₂浓度减小时谱线强度呈现先增强后减弱的趋势. 实验结果很好的验证了N₂第二正带系光谱理论计算的正确性.     

15N216O在1650-3450 cm-1的高分辨红外光谱

采用傅里叶变换红外光谱仪记录了富含¹⁵N₂¹⁶O同位素的一氧化二氮样品在1650-3450 cm^-1波段的高分辨振转光谱,得到了该同位素分子超过7300吸收谱线位置的实验值,经分析实验精确度好于5.0×10^-4 cm^-1. 基于有效哈密顿量模型预测和带带转动分析,确定了所有吸收线的归属;获得了29个新吸收带的振转光谱参数,并优化了其他44个吸收带的光谱参数值. 并且发现有效哈     

氮分子离子A2Πu-X2Σ+g 带系转动光谱分析:

利用光外差速度调制分子光谱技术测得氮分子离子A²Π_u-X²Σ⁺_g 带系的(3,1)、(4,2)、(5,3)、(8,5)带的谱线,其中(5,3)带是第一次被指认．利用测得的4个带以及文献中的14个带的谱线进行全局拟合,得到了一系列的分子常数(υ_A=0～9和υ_A=0～5)．     

精确预言双原子分子Q线系高振转激发态的跃迁谱线

用多重差分的方法,从双原子分子跃迁谱线的普遍表达式出发,已经建立起了预言双原子分子P线系高激发振转跃迁谱线的解析物理公式。采用同样的方法,充分利用现有实验条件下测定的部分振转跃迁谱线数据,文章建立了预言双原子分子Q线系高激发振转跃迁谱线的物理公式。使用该公式和一组经过物理筛选的(15条)精确的实验跃迁谱线,研究了IrN分子A1Π—X1Σ+跃迁系统中(4,1),(3,1)跃迁带的Q支发射光谱。结果表明,该公式不仅很好地重复了所有已知的实验光谱数据,且正确预言了实验没有获得的很多高转动量子态的未知发射谱线,从而提供了一种新的预言高转动量子态的未知跃迁谱线的物理方法。     

VN分子R线系跃迁结构的研究与分析

本文借助孙卫国课题组建立的能精确计算双原子分子R线系发射谱线的物理公式,利用实验上获得的低振动态跃迁谱线数据研究了电极材料VN分子电子态f¹Φ–a¹Δ以及电子态d¹∑⁺–X³Δ₁等跃迁体系的（0,0）跃迁带的R线系发射谱线. 从理论上预言了实验上难以获得的该跃迁带R线系高振转激发态的跃迁结构,为急需VN分子内部结构的其他研究领域提供了重要的结构信息. 从这些公式出发,我们定义了表征实验测定谱线对新谱线的贡献度C（contribution）参数,进一步分析了高激发振转跃迁谱线的相互依赖关系,结果表明该物理公式不仅很好地复现了已知的实验数据,正确地预言了实验未能测定的高激发振转跃迁谱线,而且还能了解不同实验谱线对新谱线的贡献程度,基于这些贡献度,实验学家可以将有限的资源更好地进行分配,重点研究那些贡献度大的振转跃迁谱线. 关键词： 双原子分子 跃迁谱线 贡献度 VN     

Self-broadening, self-shift and self-mixing in the ν2, 2ν2 and ν4 bands of NH3

Using Fourier-transform spectra (Bruker IFS 120 HR, resolution ≈0.004 cm⁻¹) of NH₃ in nine branches of the ν₂, 2ν₂ and ν₄ bands, self-broadening and self-shift as well as self-mixing coefficients have been determined at room temperature (T=295 K) for more than 350 rovibrational lines located in the spectral range 1000–1800 cm⁻¹. A non-linear least-squares multispectrum fitting procedure, including line mixing effects, has been used to retrieve successively the line parameters from 11 experimental spectra recorded at different pressures of pure NH₃. The accuracies of self-broadening coefficients are estimated to be better than 2% for most lines. The mean accuracies of line-mixing and line-shift data are estimated to be about 15% and 25%, respectively. The results are compared with previous measurements and with values calculated using a semiclassical model based upon the Robert–Bonamy formalism that reproduces rather well the systematic experimental J and K quantum number dependencies of the self-broadening coefficients.The results concerning line mixing demonstrate a large amount of coupling between the symmetric and asymmetric components of inversion doublets mainly in the ν₄ band. The line mixing parameters are both positive and negative. More than two thirds of the lines studied here have a positive shift coefficient. However, for most of them the shift coefficients are negative in the 2ν₂ band. They are positive for the R branch of the ν₂ band and for the ^PR and ^RP branches of the ν₄ band. For the other branches they are both positive and negative. Some components of inversion doublets illustrate a correlation between line mixing and shift phenomena demonstrated by a quadratic pressure dependence of line position.     

The radiative characteristics of the rovibronic states of the hydrogen molecule: IV. Relative probabilities of the r 3Π g ? , s 3Δ g ? → c 3Π u ± spontaneous transitions of the H2 molecule

A statistical analysis of the available literature data and data obtained in this work on the wave numbers of the lines that appear in triplet-triplet rovibronic transitions of the H₂ molecule was performed. This allowed us to verify and refine the controversial identification of spectral lines and find the optimum rovibronic level energy values for the c ³Π _u ^±, r ³Π _g ⁻, and s ³Δ _g ⁻ states. The ratios between the line strengths of the P, Q, and R branches of the (4dπ)r ³Π _g ⁻, (4dδ)s ³Δ _g ⁻ → (2pπ)c ³Π _u ^± band systems of the H₂ molecule were measured systematically. The calculation results obtained in the Frank-Condon approximation differed substantially (by up to two orders of magnitude) from the experimental data. The dependences of the ratios between rovibronic line strengths of the r ³Π _g ⁻ → c ³Π _u ^± and s ³Δ _g ⁻ → c ³Π _u ^± transitions on the rotational quantum number N′ of the upper level were found to correlate with each other. The deviations of adiabatic theory increase as N′ grows, which is evidence of an important role played by electronic-rotational interactions in the perturbation of transition probabilities. The experimental ratios between the probabilities of rovibronic transitions satisfactorily agree with the results of calculations within the framework of the simple nonadiabatic model taking into account electronic-rotational interaction of radiating adiabatic states in the approximation of pure precession. The dependences of transition probabilities on N′ were obtained for the first time for the first four diagonal bands of the r ³Π _g ⁻, s ³Δ _g ⁻ → c ³Π _u ^± transitions. Original Russian Text ? S.A. Astashkevich, B.P. Lavrov, A.V. Modin, I.S. Umrikhin, 2008, published in Khimicheskaya Fizika, 2008, Vol. 27, No. 2, pp. 22–38.     

Postcollision interaction upon electron excitation of 4sns1S0, 3S1 and 4snd1D2, 3DJ levels of zinc atom

The optical excitation functions (OEFs) for four series of spectral lines of the Zn atom at the transitions 4sn ₁ s ¹ S ₀ → 4s4p ¹ P ₁^∘ (n ₁ = 6–10), 4sn ₂ s ³ S ₁ → 4s4p ³ P ₂^∘ (n ₂ = 6−8), 4sn ₃ d ¹ D ₂ → 4s4p ¹ P ₁^∘ (n ₃ = 4−6), 4sn ₄ d ³ D _{1, 2, 3} → 4s4p ³ P ₂^∘ (n ₄ = 4−7) excited by a monoenergetic (0.04–0.08 eV) electron beam with energies from the excitation threshold to 18–19 eV are measured. In the energy dependences of the excitation cross sections, the effect of post-collision interaction of slow (scattered) and fast (emitted after the autoionization state decay) electrons is observed and described. This interaction leads to the capture of a slow electron into the listed discrete levels and the appearance of maxima in the excitation functions. The energies of the maxima are used to determine the energies and widths of single autoionization states or their groups by approximate formulas of the classical approach. The autoionization levels of the zinc atom responsible for the maxima observed are determined. Possible transfer of the orbital angular momentum between electrons is analyzed.     

Eu3+-based optical centers with a high efficiency of the 5D0 → 7F4 transition in alumina gel films

A record peak luminescence intensity of the ⁵ D ₀ → ⁷ F ₄ transition in Eu³⁺ ions and broadening of their UV excitation band are obtained by doping of Eu-containing alumina gel films with bismuth oxyfluoride and subsequent thermal treatment at T ≥ 700°C. The results obtained are explained by the formation of complex Eu—Bi centers with C _3V symmetry in the Al₂O₃ structure, efficient migration of excitations from EuAlO₃ crystallites to these centers, and the sensitization of the luminescence of the rare-earth activator by Bi³⁺ ions. __________ Translated from Optika i Spektroskopiya, Vol. 98, No. 2, 2005, pp. 224–228. Original Russian Text Copyright ? 2005 by Malashkevich, Shevchenko, Bokshits, Kornienko, Pershukevich.     

NH3 self-broadening coefficients in the ν2 and ν4 bands and line intensities in the ν2 band

Self-broadening coefficients of NH₃ in the ν₂ and ν₄ bands and absolute line intensities in the ν₂ band have been measured at room temperature for some selected lines in the P- and R-branches. Using a Fourier transform spectrometer, line intensities and collisional widths were obtained by fitting Voigt profiles to the measured shapes of the lines. The results of self-broadening coefficients are in reasonable agreement with calculated linewidths using a semiclassical model which reproduce rather well the systematic experimental J and K quantum numbers dependencies. Satisfactory agreement was also obtained for line intensities with previous measurements in the ν₂ band. From the intensity measurements, we have determined effective transition dipole moments as well as Herman–Wallis parameters for the ν₂ band.     

Contribution to the Analysis of theA2←XA1“Wulf” Transition of Ozone by High-Resolution Fourier Transform Spectrometry

The analysis of the rotational structure of the high-resolution Fourier transform 0⁰₀absorption spectrum of the³A₂←X¹A₁band system of the “Wulf” transition of the isotopomer¹⁶O₃of ozone is reported for the first time. With a near pure case (b) coupling model for the upper triplet state, we have assigned a significant portion of the spectrum, mainly theF₁(J=N+ 1) andF₂(J=N) spin components, primarily in the lower frequency region of the band. The lines corresponding to theF₃(J=N− 1) component are weak at lower frequencies and heavily congested in the central and higher frequency regions of the spectrum. Perturbations and predissociation phenomena have reduced the effective lifetime of the metastable³A₂state and have also limited the number of transitions included in the least-squares fit of the band. Approximately 100 lines have been assigned in the range from 9100–9550 cm⁻¹. Three rotational, three centrifugal distortion, three spin–rotation, and one spin–spin constant were varied. The geometry of the molecule in the³A₂state, as determined from these constants, isr= 1.345 Å and θ = 98.9°, in good agreement withab initioresults.     

Line strength measurements of carbonyl sulfide (OCS) in the 2v3, v1+2v2+v3, and 4v2+v3 bands

To support planetary studies of the Venus atmosphere, we measured line strengths of the 2v₃, v₁+2v₂+v₃, and 4v₂+v₃ bands of the primary isotopologue of carbonyl sulfide (¹⁶O¹²C³²S), whose band centers are located at 4101.387, 3937.427, and 4141.212 cm⁻¹, respectively. For this, infrared absorption spectra in normal carbonyl sulfide (OCS) sample gas were recorded at an unapodized resolution of 0.0033 cm⁻¹ at ambient room temperatures using a Bruker Fourier transform spectrometer (FTS) at the Jet Propulsion Laboratory. The FTS instrumental line shape (ILS) function was investigated, which revealed no significant instrumental line broadening or distortions. Various custom-made short cells and a multi-pass White cell were employed to achieve optical densities sufficient to observe the strong 2v₃ and the weaker bands in the region. Gas sample impurities and the isotopic abundances were determined from mass spectrum analysis. Line strengths were retrieved spectrum by spectrum using a non-linear curve fitting algorithm adopting a standard Voigt line profile, from which Herman–Wallis factors were derived for the three bands. The band strengths of 2v₃, v₁+2v₂+v₃, and 4v₂+v₃ of ¹⁶O¹²C³²S (normalized at 100% of isotopologue) are observed to be 6.315(13)×10⁻¹⁹, 1.570(2)×10⁻²⁰, and 7.949(20)×10⁻²¹ cm⁻¹/molecule cm⁻², respectively, at 296 K. These results are compared with earlier measurements and the HITRAN 2004 database.     

The 2ν8 Band of CH3CN

The overtone band 2ν⁰₈ of CH₃CN around 720 cm⁻¹ has been measured on a Bruker Fourier transform spectrometer at a resolution of 0.003 cm⁻¹. Only the parallel band was observed, but due to the l(2, 2) resonance, ΔK = −2 lines leading to the v₈ = 2, l₈ = −2 levels with K = 1-3 could be seen. More information for the l₈ = ±2 component of the vibrational state v₈ = 2 was evaluated from the hot band 2ν^±2₈ - ν^±1₈. Altogether more than 1000 lines were assigned. In the fit pure rotational lines from literature were also combined. Among the results the anomalous A₀ - A′ values 4.6722(13) × 10⁻³ cm⁻¹ for the 2ν⁰₈ band and 7.0324(32) × 10⁻³ cm⁻¹ for the 2ν^±2₈ band are striking.     

High-resolution FTIR spectroscopy of HNSO—Analysis of the highly perturbed ν4, ν6 and 2ν5 bands

We report a rovibrational analysis of the ν₄ and ν₆ fundamentals and the 2ν₅ overtone of HNSO from high-resolution Fourier transform infrared spectra. The ν₆ band (out-of-plane bend) centred at 757.5 cm⁻¹ is c-type. The ν₄ band (HNS bend) centred at 905.9 cm⁻¹ is predominantly a-type with a very weak b-type component (). Numerous global perturbations and localized avoided crossings affecting the v₄ = 1 rotational levels were successfully treated by inclusion of Fermi and c-axis Coriolis resonance terms between v₄ = 1 and v₅ = 2, and a b-axis Coriolis resonance term between v₄ = 1 and v₆ = 1. The latter term gives rise to an avoided crossing with an extraordinary ΔK_a = 5 selection rule. The Fermi resonance between v₄ = 1 and v₅ = 2 gives rise to strong mixing of their rotational wavefunctions in the vicinity of K_a = 18. The resultant borrowing of intensity made it possible for 2ν₅ transitions in the range K_a = 16–19 to be assigned and included in a global rovibrational treatment of all three band systems.