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arXiv 1609.00403physics.atom-phastro-ph.HEastro-ph.IM
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Si和S L壳层离子K壳层跃迁能的实验室测量

Laboratory Measurements of the K-shell transition energies in L-shell ions of Si and S

N. Hell, G. V. Brown, J. Wilms, V. Grinberg, J. Clementson, D. Liedahl, F. S. Porter, R. L. Kelley, C. A. Kilbourne, P. Beiersdorfer

摘要:

我们用劳伦斯利弗莫尔国家实验室的电子束离子阱EBIT-Ⅰ和SuperEBIT以及NASA/GSFC EBIT量热谱仪(ECS)测量了He ~--类Ne硅和硫离子中最强的1 s-2 ell(ell=s,p)跃迁的能量,精确度优于1 eV。我们确定和测量的能量18和21 X射线的功能,分别从硅和硫。结果与新的灵活原子代码计算和Palmeri等人(2008)的半相对论Hartree Fock计算进行了比较。这些结果对于高质量X射线双星(如船帆座X-1和天鹅座X-1)的风诊断特别有用,在这些双星中,使用钱德拉的高能透射光栅进行的高分辨率光谱测量使测量100 km/s的多普勒频移成为可能。我们的测量精度与分析钱德拉观测所需的精度一致,超过了钱德拉100 km/s的极限。因此,这里给出的结果不仅提供了理论基准,而且还提供了精确的静止能量,可用于确定天体物理源中物质的整体运动。我们表明,我们的结果的有用性,通过应用它们来重新确定多普勒频移从钱德拉观测船帆座X-1。

英文摘要:

We have measured the energies of the strongest 1s-2ell (ell=s,p) transitions in He- through Ne-like silicon and sulfur ions to an accuracy of better than 1eV using Lawrence Livermore National Laboratory's electron beam ion traps, EBIT-I and SuperEBIT, and the NASA/GSFC EBIT Calorimeter Spectrometer (ECS). We identify and measure the energies of 18 and 21 X-ray features from silicon and sulfur, respectively. The results are compared to new Flexible Atomic Code calculations and to semi-relativistic Hartree Fock calculations by Palmeri et al. (2008). These results will be especially useful for wind diagnostics in high mass X-ray binaries, such as Vela X-1 and Cygnus X-1, where high-resolution spectral measurements using Chandra's high energy transmission grating has made it possible to measure Doppler shifts of 100km/s. The accuracy of our measurements is consistent with that needed to analyze Chandra observations, exceeding Chandra's 100km/s limit. Hence, the results presented here not only provide benchmarks for theory, but also accurate rest energies that can be used to determine the bulk motion of material in astrophysical sources. We show the usefulness of our results by applying them to redetermine Doppler shifts from Chandra observations of Vela X-1.

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