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High resolution spectroscopy of jet cooled phenyl radical: The nu(1) and nu(2) a(1) symmetry C-H stretching modes

机译:喷射冷却的苯基自由基的高分辨率光谱:nu(1)和nu(2)a(1)对称C-H拉伸模式

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A series of CH stretch modes in phenyl radical (C6H5) has been investigated via high resolution infrared spectroscopy at sub-Doppler resolution (similar to 60 MHz) in a supersonic discharge slit jet expansion. Two fundamental vibrations of a(1) symmetry, nu(1) and nu(2), are observed and rotationally analyzed for the first time, corresponding to in-phase and out-of-phase symmetric CH stretch excitation at the ortho/meta/para and ortho/para C atoms with respect to the radical center. The nu(1) and nu(2) band origins are determined to be 3073.968 50(8) cm(-1) and 3062.264 80(7) cm(-1), respectively, which both agree within 5 cm(-1) with theoretical anharmonic scaling predictions based on density functional B3LYP/6-311g++(3df,3dp) calculations. Integrated band strengths for each of the CH stretch bands are analyzed, with the relative intensities agreeing remarkably well with theoretical predictions. Frequency comparison with previous low resolution Ar-matrix spectroscopy [A. V. Friderichsen et al., J. Am. Chem. Soc. 123, 1977 (2001)] reveals a nearly uniform Delta nu approximate to + 10-12 cm(-1) blue shift between gas phase and Ar matrix values for nu(1) and nu(2). This differs substantially from the much smaller red shift (Delta nu approximate to -1 cm(-1)) reported for the nu(19) mode, and suggests a simple physical model in terms of vibrational mode symmetry and crowding due to the matrix environment. Finally, the infrared phenyl spectra are well described by a simple asymmetric rigid rotor Hamiltonian and show no evidence for spectral congestion due to intramolecular vibrational coupling, which bodes well for high resolution studies of other ring radicals and polycyclic aromatic hydrocarbons. In summary, the combination of slit jet discharge methods with high resolution infrared lasers enables spectroscopic investigation of even highly reactive combustion and interstellar radical intermediates under gas phase, jet-cooled (T-rot approximate to 11 K) conditions.
机译:在超音速放电狭缝射流扩展中,已通过亚多普勒分辨率(类似于60 MHz)下的高分辨率红外光谱研究了苯基自由基(C6H5)中的一系列CH拉伸模式。首次观察到两个a(1)对称的基本振动nu(1)和nu(2)并进行旋转分析,分别对应于正交/元相的同相和异相对称CH拉伸激励相对于自由基中心的/ para和ortho / para C原子。 nu(1)和nu(2)的波段起点分别确定为3073.968 50(8)cm(-1)和3062.264 80(7)cm(-1),两者均在5 cm(-1)内基于密度泛函B3LYP / 6-311g ++(3df,3dp)计算的理论非谐比例缩放预测。分析了每个CH拉伸带的综合带强度,其相对强度与理论预测非常吻合。与以前的低分辨率Ar矩阵光谱法进行频率比较[A. V.Friderichsen等,J.Am。化学Soc。 123,1977(2001)]揭示了在nu(1)和nu(2)的气相和Ar矩阵值之间的近似均匀的Delta nu接近+ 10-12 cm(-1)蓝移。这与nu(19)模式报道的小得多的红移(Delta nu近似于-1 cm(-1))完全不同,并建议了一个简单的物理模型,涉及振动模式的对称性和基质环境引起的拥挤。最后,一个简单的非对称刚性转子哈密顿量很好地描述了红外苯基光谱,并且没有显示出由于分子内振动耦合而引起的光谱拥塞的证据,这对于其他环基和多环芳烃的高分辨率研究而言是一个好兆头。总而言之,狭缝喷射放电方法与高分辨率红外激光的结合使得在气相,喷射冷却(T-rot约11 K)条件下,即使是高反应性燃烧和星际自由基中间体也能进行光谱研究。

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