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Experimental and theoretical study of line mixing in methane spectra. I. The N_2-broadened v_3 band at room temperature

机译:甲烷谱线混合的实验和理论研究。一,室温下N_2展宽的v_3带

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Line-mixing effects have been studied in the v_3 band of CH_4 perturbed by N_2 at room temperature. New measurements have been made and a model is proposed which is not, for the first time, strictly empirical. Three different experimental set ups have been used in order to measure absorption in the 2800-3200 cm~(-1) spectral region for total pressures in the 0.25-2 and 25-80 atm ranges. Analysis of the spectra demonstrates the significant influence of line mixing on the shape of the Q branch and of the P and R manifolds. A model is proposed which is based on state-to-state collisional transfer rates calculated from the intermolecular potential surface with a semiclassical approach. The line-coupling relaxation matrix is constructed from these data and two additional parameters which are fitted on measured absorption. Comparisons between measurements and spectra computed accounting for and neglecting line mixing are made. They prove the quality of the approach which satisfactory accounts for the effects of pressure and of rotational quantum numbers on the spectral shape under conditions where modifications introduced by line mixing are important. For high rotational quantum number lines, the main features induced by collisions are predicted but some discrepancies remain; The latter may be due to improper line-coupling elements but there is strong evidence that the use of inaccurate line broadening parameters also contributes to errors in calculated spectra.
机译:在室温下,在CH_4的v_3波段被N_2扰动时研究了线混合效应。已经进行了新的测量,并提出了一个首次不是严格基于经验的模型。为了测量0.25-2和25-80 atm范围内的总压力,已使用三个不同的实验装置来测量2800-3200 cm〜(-1)光谱区域中的吸收。光谱分析表明,线路混合对Q支路以及P和R歧管的形状有重大影响。提出了一种模型,该模型基于使用半经典方法从分子间势能表面计算出的状态间碰撞转移速率。线耦合弛豫矩阵由这些数据和两个附加参数构成,这些参数适合于测量的吸收。进行了测量值和频谱计算值之间的比较,以说明并忽略了线路混合。他们证明了这种方法的质量,该方法可以令人满意地说明在压力混合和线混合引起的重要变化条件下,压力和旋转量子数对光谱形状的影响。对于高旋转量子数线,可以预测由碰撞引起的主要特征,但仍存在一些差异。后者可能是由于线路耦合元素不当引起的,但是有充分的证据表明,使用不正确的线路加宽参数也会导致计算光谱中的误差。

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