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用于天体物理电荷交换等离子体建模的原子数据中的不确定性。

Uncertainties in Atomic Data for Modeling Astrophysical Charge Exchange Plasmas.

作者信息

Gu Liyi, Shah Chintan, Zhang Ruitian

机构信息

SRON Netherlands Institute for Space Research, Niels Bohrweg 4, 2333 CA Leiden, The Netherlands.

RIKEN High Energy Astrophysics Laboratory, 2-1 Hirosawa, Wako 351-0198, Saitama, Japan.

出版信息

Sensors (Basel). 2022 Jan 19;22(3):752. doi: 10.3390/s22030752.

Abstract

Relevant uncertainties of theoretical atomic data are vital to determining the accuracy of plasma diagnostics in a number of areas, including, in particular, the astrophysical study. We present a new calculation of the uncertainties on the present theoretical ion-impact charge exchange atomic data and X-ray spectra, based on a set of comparisons with the existing laboratory data obtained in historical merged-beam, cold-target recoil-ion momentum spectroscopy, and electron beam ion traps experiments. The average systematic uncertainties are found to be 35-88% on the total cross sections, and 57-75% on the characteristic line ratios. The model deviation increases as the collision energy decreases. The errors on total cross sections further induce a significant uncertainty to the calculation of ionization balance for low-temperature collisional plasmas. Substantial improvements of the atomic database and dedicated laboratory measurements are needed to obtain the current models, ready for the X-ray spectra from the next X-ray spectroscopic mission.

摘要

理论原子数据的相关不确定性对于确定许多领域中(特别是天体物理研究领域)等离子体诊断的准确性至关重要。我们基于与历史合并束、冷靶反冲离子动量谱和电子束离子阱实验中获得的现有实验室数据的一组比较,对当前理论离子碰撞电荷交换原子数据和X射线光谱的不确定性进行了新的计算。发现总截面的平均系统不确定性为35% - 88%,特征线比的平均系统不确定性为57% - 75%。模型偏差随着碰撞能量的降低而增加。总截面的误差进一步给低温碰撞等离子体的电离平衡计算带来了显著的不确定性。需要大幅改进原子数据库并进行专门的实验室测量,以使当前模型适用于下一次X射线光谱任务的X射线光谱。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4ecc/8839592/768065bc8421/sensors-22-00752-g001.jpg

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