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首页> 外文期刊>The Journal of Chemical Physics >A mass and time-of-flight spectroscopy study of the formation of clusters in free-jet expansions of normal D_2
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A mass and time-of-flight spectroscopy study of the formation of clusters in free-jet expansions of normal D_2

机译:质量和飞行时间光谱研究正常D_2自由喷射膨胀中团簇的形成

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摘要

The mass spectra in the range of 2(D~+)-38(D_(19)~+) amu of clusters formed in a supersonic free-jet expansion of normal D_2 are investigated as functions of source temperature in the range of 95-220 K and of source pressure in the range of 10-120 bars.For some of the small ion fragments,time-of-flight distributions are also measured.For large clusters (n>200) the intensities of the odd-numbered ion fragments exhibit magic numbers at D_9~+and D_(15)~+in accordance with previous experiments and calculations.The even-numbered ion fragments have much smaller intensities and exhibit new magic numbers at D_(10)~+and D_(14)~+.For source conditions such that large clusters are formed,the intensities of the various different ion fragments are observed to saturate beyond a certain source pressure.At lower source pressures,where only small clusters are formed,the terminal mole fractions of the neutral dimers are analyzed in the light of available theories which take into account both the thermodynamics and the kinetics of the expansion.At higher source pressures and lower temperatures,where larger clusters are formed,the sizes of the neutral clusters are estimated using scaling laws and are found to be consistent with the mass spectra and measured time-of-flight distributions.By using a variety of techniques it has been possible to obtain reliable conclusions about the neutral cluster sizes for the present free-jet expansion conditions.
机译:研究了在正常D_2的超音速自由射流扩展中形成的簇的2(D〜+)-38(D_(19)〜+)amu范围内的质谱与源温度在95- 220 K,源压在10-120 bar范围内。对于一些小离子碎片,还测量了飞行时间分布;对于大簇(n> 200),奇数离子碎片的强度根据先前的实验和计算,在D_9〜+和D_(15)〜+处显示幻数。偶数离子碎片的强度小得多,在D_(10)〜+和D_(14)〜处显示新的幻数。 +。对于形成大簇的离子源条件,观察到各种不同离子碎片的强度超过一定的离子源压力会饱和。在较低的离子源压力下,仅形成小簇的中性二聚体的末端摩尔分数根据可用的理论进行分析,这些理论同时考虑了在较高的源压力和较低的温度下,形成较大的团簇,使用比例定律估算中性团簇的大小,发现它们与质谱和测量的飞行时间一致通过使用多种技术,有可能获得关于当前自由射流膨胀条件下中性星团大小的可靠结论。

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