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采用时间切片速度成像光电离质谱(TS-VMI-PI-MS)技术测定态选择光解 N 产生的 N(D)和 N(D)自旋轨道态分支比。

Branching Ratios of the N(D) and N(D) Spin-Orbit States Produced in the State-Selected Photodissociation of N Determined Using Time-Sliced Velocity-Mapped-Imaging Photoionization Mass Spectrometry (TS-VMI-PI-MS).

机构信息

Department of Chemistry , University of California , Davis , California 95616 , United States.

Wuhan Institute of Physics and Mathematics, CAS , Wuhan 430071 , China.

出版信息

J Phys Chem A. 2019 Mar 28;123(12):2289-2300. doi: 10.1021/acs.jpca.8b11691. Epub 2019 Feb 4.

DOI:10.1021/acs.jpca.8b11691
PMID:30628443
Abstract

Branching ratios for N(D) and N(D) produced by predissociation of state selected excited nitrogen molecules in the vacuum ultraviolet region have been measured for the first time. The quantum numbers of the excited nitrogen molecule are defined by selective excitation of the nitrogen molecule in the Franck-Condon region from the ground electronic, Σ, vibrational, v″, and rotational, J″ state to an excited E', v', J' state with a tunable vacuum ultraviolet, VUV, laser. The neutral atoms produced by predissociation from this excited state are then selectively ionized with a second tunable VUV laser. Measurement of the relative populations of these two atoms formed in their spin-orbit states defines the quantum states for the atomic products. This means that the wave functions of the initial state and knowledge of the relative yields define all the experimental parameters for this series of unimolecular reactions. The ions formed by VUV are mass analyzed with a time-of-flight mass spectrometer and detected with a time slice velocity ion imaging mass spectrometer. In this manner, we can determine the recoil velocity associated with the predissociation process. Two different techniques are used to determine the spin-orbit ratios, namely, resonant VUV photoionization (RVUV-PI) spectroscopy and total kinetic energy release (TKER) spectroscopy determined from the image produced when the atoms are selectively ionized by VUV in the interaction region. The TKER spectra obtained from the lines at 110 296.25 and 110 304.96 cm that couple to a newly discovered autoionization line at 129 529.4255 ± 0.0015 cm prove that the lines observed in this region originate from the N(D) and N(D) atoms. Two other lines in this region at 110 286.20 and 110 299.89 cm originate from the nitrogen N(S) that is photoionized in a 1+ 1 VUV-UV resonant multiphoton ionization process. The spin-orbit branching ratios have been evaluated for valence and Rydberg electronic excited states from 104 129.4 to 118 772.1 cm, and it shows that they are independent of the rotational and vibrational quantum numbers. They are not appreciably affected by the symmetry properties of the wave function in the Franck-Condon region of the excited states. In the energy region below 117 153.8 cm the pathways at long internuclear distances appear to determine [N(D)]/[N(D)] branching ratios of ∼0.38, ∼0.62, and ∼1.04. At higher energies, TKER and RVUV-PI spectroscopy have been used to show that the average fraction of the N(D) and N(D) atoms produced in the spin-allowed channels that produce two N(D) is 0.85 versus 0.15 for spin-forbidden channels. The importance and need for this information for comparison with theory and applications in astrochemistry are briefly discussed.

摘要

首次测量了在真空紫外区预解离状态选择激发氮分子产生的 N(D)和 N(D)的分支比。通过可调谐真空紫外(VUV)激光从基电子Σ、振动 v″和转动 J″态选择性激发 Franck-Condon 区域中的氮分子,定义了激发氮分子的量子数到一个激发的 E'、v'、J'态。通过第二可调谐 VUV 激光预解离从该激发态产生的中性原子随后被选择性离子化。测量这两种原子在其自旋轨道态中形成的相对丰度,定义原子产物的量子态。这意味着初始态的波函数和相对产率的知识定义了这一系列单分子反应的所有实验参数。通过飞行时间质谱仪对 VUV 形成的离子进行质量分析,并通过时间切片速度离子成像质谱仪进行检测。通过这种方式,我们可以确定与预解离过程相关的反冲速度。使用两种不同的技术来确定自旋轨道比,即通过 VUV 在相互作用区域选择性离子化时产生的共振 VUV 光致电离 (RVUV-PI) 光谱和总动能释放 (TKER) 光谱。从原子在该区域中通过 VUV 选择性离子化时产生的图像中确定的 TKER 光谱,证明在该区域中观察到的线源自 N(D)和 N(D)原子。该区域中的另外两条线,在 110286.20 和 110299.89 cm,源自氮 N(S),它在 1+1 VUV-UV 共振多光子电离过程中被光致电离。从 104129.4 到 118772.1 cm,评估了价电子和里德伯电子激发态的自旋轨道分支比,结果表明它们与转动和振动量子数无关。它们不受激发态 Franck-Condon 区域中波函数的对称性的影响。在低于 117153.8 cm 的能量区域中,长核间距离的途径似乎决定了[N(D)]/[N(D)]分支比约为 0.38、0.62 和 1.04。在更高的能量下,TKER 和 RVUV-PI 光谱已被用于表明在自旋允许通道中产生两个 N(D)的 N(D)和 N(D)原子的平均分数为 0.85,而对于自旋禁止通道则为 0.15。简要讨论了这些信息对于与天体化学中的理论和应用进行比较的重要性和必要性。

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