论文标题

NE,CO $ _2 $和SF $ _6 $的软X射线过渡能的新基准:铺平通往PPM精度的途径

A new benchmark of soft X-ray transition energies of Ne, CO$_2$, and SF$_6$: paving a pathway towards ppm accuracy

论文作者

Stierhof, J., Kühn, S., Winter, M., Micke, P., Steinbrügge, R., Shah, C., Hell, N., Bissinger, M., Hirsch, M., Ballhausen, R., Lang, M., Gräfe, C., Wipf, S., Cumbee, R., Betancourt-Martinez, G. L., Park, S., Niskanen, J., Chung, M., Porter, F. S., Stöhlker, T., Pfeifer, T., Brown, G. V., Bernitt, S., Hansmann, P., Wilms, J., López-Urrutia, J. R. Crespo, Leutenegger, M. A.

论文摘要

正确解释高分辨率X射线光谱的关键要求是,过渡能的精度和精确度很高。我们通过同时测量其在北极X Ebit中产生的He-like离子的1S-NP荧光发射的He-like IOMS的贝西II同步器功能,研究NE,CO $ _2 $和SF $ _6 $气体的K-shell功能。这些离子中过渡的准确计算提供了校准的基础。尽管Co $ _2 $结果与以前的测量非常吻合,但SF $ _6 $频谱似乎转移了〜0.5 eV,大约是早期结果的不确定性的两倍。我们的NE结果显示出与早期结果的差异很大,但可能比其他测量值更大。分子光谱与我们时间依赖性密度功能理论的结果非常吻合。我们发现统计不确定性允许在1-10 MEV范围内进行校准,但是,系统的贡献仍将不确定性限制为〜40-100 MEV,这主要是由于单色能量量表的时间稳定性。将我们的绝对校准技术与相对能量校准技术(例如光电子能量光谱)相结合,以实现其达到低至1-10 MEV的不确定性的全部潜力。

A key requirement for the correct interpretation of high-resolution X-ray spectra is that transition energies are known with high accuracy and precision. We investigate the K-shell features of Ne, CO$_2$, and SF$_6$ gases, by measuring their photo ion-yield spectra at the BESSY II synchrotron facility simultaneously with the 1s-np fluorescence emission of He-like ions produced in the Polar-X EBIT. Accurate ab initio calculations of transitions in these ions provide the basis of the calibration. While the CO$_2$ result agrees well with previous measurements, the SF$_6$ spectrum appears shifted by ~0.5 eV, about twice the uncertainty of the earlier results. Our result for Ne shows a large departure from earlier results, but may suffer from larger systematic effects than our other measurements. The molecular spectra agree well with our results of time-dependent density functional theory. We find that the statistical uncertainty allows calibrations in the desired range of 1-10 meV, however, systematic contributions still limit the uncertainty to ~40-100 meV, mainly due to the temporal stability of the monochromator energy scale. Combining our absolute calibration technique with a relative energy calibration technique such as photoelectron energy spectroscopy will be necessary to realize its full potential of achieving uncertainties as low as 1-10 meV.

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