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High resolution emission Fourier transform infrared spectra of the 4p-5s and 5p-6s bands of ArH

机译:ArH 4p-5s和5p-6s波段的高分辨率发射傅里叶变换红外光谱

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In the 2500-8500 cm(-1) region several strong emission bands of (ArH)-Ar-40 were observed by Fourier transform spectroscopy through a dc glow discharge in a mixture of argon and hydrogen. Rotational-electronic, transitions of the two previously unstudied 4p-5s and 5p-6s, nu = 0-0, bands of (ArH)-Ar-40 were measured and assigned in the 6060 and 3770 cm-1 regions, respectively. A simultaneous fit of the emission transitions of the 4p-5s and 5p-6s bands and an extended set of transitions of the 6s-4p band observed by Dabrowski, Tokaryk, and Watson [J. Mol. Spectrosc. 189, 95 (1998)] and remeasured in the present work yielded consistent values of the spectroscopic parameters of the electronic states under investigation. In the branch of the 4p-5s band with transitions of type (Q)Q(f3e) we observed a narrowing in the linewidths with,increasing rotational quantum number N. The rotational dependence of the linewidth is caused by predissociation of the 5s state by the repulsive ground 4s state through. homogeneous coupling and changes in overlap integrals of the vibrational wave functions with the rotational level. Analysis was based on the. Fermi's golden rule approximation model. In. the 4p-5s band region a vibrational sequence of nu'-nu ''= 1-1, 2-2, and 3-3 were recorded and a number of transitions belonging to the strongest (Q)Q(f3e) form branch of the 1-1 band were analyzed. (c) 2005 American Institute of Physics.
机译:在2500-8500 cm(-1)区域中,通过在氩气和氢气的混合物中进行的直流辉光放电,通过傅里叶变换光谱法观察到(ArH)-Ar-40的几个强发射带。分别在6060和3770 cm-1区域测量并分配了两个先前未研究的4p-5s和5p-6s(nu = 0-0)(ArH)-Ar-40的旋转电子跃迁。 Dabrowski,Tokaryk和Watson观察到4p-5s和5p-6s波段的发射跃迁同时拟合和6s-4p波段的跃迁扩展集[J.大声笑光谱。 189,95(1998)],并在本工作中重新测量,得出了所研究电子态的光谱参数的一致值。在具有(Q)Q(f3e)类型跃迁的4p-5s波段的分支中,我们观察到随着旋转量子数N的增加,线宽变窄。线宽的旋转依赖性是由5s状态的预解离引起的。排斥地面4s通过。均匀耦合以及振动波函数的重叠积分随旋转水平的变化。分析依据。费米的黄金法则近似模型。在。记录了4p-5s波段区域的振动序列nu'-nu''= 1-1、2-2和3-3,并且属于最强(Q)Q(f3e)形式分支的许多跃迁对1-1频段进行了分析。 (c)2005年美国物理研究所。

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