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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的自由射流膨胀中团簇的形成

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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. (c) 2006 American Institute of Physics.
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在2(D +)-38(D-19(+))amu范围内的质谱与源温度在95- 220 K,源压力在10-120 bar范围内。对于某些小离子碎片,还测量了飞行时间分布。对于大型簇(n> 200),根据先前的实验和计算,奇数离子片段的强度在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(+)处显示出新的幻数。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某个离子源压力会饱和。在较低的源压力下,仅形成小团簇,根据现有理论分析中性二聚体的末端摩尔分数,该理论同时考虑了热力学和膨胀动力学。在较高的源压力和较低的温度下(其中会形成较大的星团),使用比例定律估算中性星团的大小,发现它们与质谱和测得的飞行时间分布一致。通过使用各种技术,有可能获得有关当前自由射流膨胀条件下中性星团尺寸的可靠结论。 (c)2006年美国物理研究所。

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