The nature of the absorption bandshape density evolution for the first overtone of CO compressed by N2

G.V. Tchlenova , A.A. Vigasin , J.-P. Bouanich , C. Boulet
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引用次数: 4

Abstract

Infrared spectra of the 2←0 absorption band of CO, compressed by N2 at various densities up to 220 amagat at about 296 and 187 K have been analyzed. To interpret these spectra a line-by-line model has been applied, based on empirical corrections of the Lorentzian line-shape, which account roughly for the effects of line-mixing and the finite duration of collisions. At room temperature, this model provides a satisfactory agreement with experimental bandshapes, especially for the lower N2 densities. At low temperature, the calculated absorption differs significantly from that observed around the band center, with a discrepancy increasing with the N2 density. This difficulty is overcome by accounting for the binary—van der Waals complexes— CO…N2 formation. The extent of these CO…N2 complexes has been estimated from two models of bandshape fitting the experimental profiles and by a simple thermodynamic calculation.

N2压缩CO的第一泛音吸收带形密度演化性质
在296和187k下,用不同密度的N2压缩CO的2←0吸收带进行了红外光谱分析。为了解释这些光谱,基于洛伦兹线形的经验修正,应用了逐线模型,该模型大致解释了线混合和有限碰撞持续时间的影响。在室温下,该模型与实验结果吻合较好,特别是在较低的N2密度下。在低温下,计算出的吸收值与在带中心周围观测到的吸收值存在显著差异,且差异随着N2密度的增大而增大。通过计算二元范德华配合物- CO…N2的形成,克服了这一困难。根据与实验曲线拟合的两种带形模型和简单的热力学计算,估计了这些CO…N2配合物的范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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