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氪401→5[3/2]电子跃迁的碰撞展宽和频移的温度依赖性。

Temperature dependence of collisional broadening and shift for the Kr 401→5[3/2] electronic transition.

作者信息

Sahoo Abinash, Zelenak Dominic, Narayanaswamy Venkateswaran

出版信息

Appl Opt. 2020 Feb 10;59(5):1438-1446. doi: 10.1364/AO.380102.

DOI:10.1364/AO.380102
PMID:32225402
Abstract

Temperature scaling of collisional broadening parameters for krypton (absorber) 401→5[3/2] electronic transition centered at 107.3 nm in the presence of major combustion species (perturber) is investigated. The absorption spectrum in the vicinity of the transition is obtained from the fluorescence due to the two-photon excitation scan of krypton. Krypton was added in small amounts to major combustion species such as , , , and air, which then heated to elevated temperatures when flowed through a set of heated coils. In a separate experimental campaign, laminar premixed flat flame product mixtures of methane combustion were employed to extend the investigations to higher temperature ranges relevant to combustion. Collisional full width half maximum (FWHM) () and shift () were computed from the absorption spectrum by synthetically fitting Voigt profiles to the excitation scans, and their corresponding temperature scaling was determined by fitting power-law temperature dependencies to the and data for each perturber species. The temperature exponents of and for all considered combustion species (perturbers) were -0.73 and -0.6, respectively. Whereas the temperature exponents of are closer to the value (-0.7) predicted by the dispersive interaction collision theory, the corresponding exponents of are in between the dispersive interaction theory and the kinetic theory of hard-sphere collisions. Comparison with existing literature on broadening parameters of NO, OH, and CO laser-induced fluorescence spectra reveal interesting contributions from non-dispersive interactions on the temperature exponent.

摘要

研究了在主要燃烧物种(扰动剂)存在的情况下,氪(吸收体)401→5[3/2]电子跃迁(中心波长为107.3 nm)的碰撞展宽参数的温度标度。跃迁附近的吸收光谱是通过氪的双光子激发扫描产生的荧光获得的。将少量氪添加到主要燃烧物种中,如 、 、 和空气,然后当它们流经一组加热线圈时加热到高温。在另一个实验中,采用甲烷燃烧的层流预混扁平火焰产物混合物,将研究扩展到与燃烧相关的更高温度范围。通过将Voigt轮廓综合拟合到激发扫描中,从吸收光谱计算碰撞半高宽(FWHM)( )和频移( ),并通过将幂律温度依赖性拟合到每种扰动剂物种的 和 数据来确定它们相应的温度标度。所有考虑的燃烧物种(扰动剂)的 和 的温度指数分别为-0.73和-0.6。虽然 的温度指数更接近色散相互作用碰撞理论预测的值(-0.7),但相应的 的指数介于色散相互作用理论和硬球碰撞动力学理论之间。与现有关于NO、OH和CO激光诱导荧光光谱展宽参数的文献比较,揭示了非色散相互作用对温度指数的有趣贡献。

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