Charge-exchange spectroscopic diagnostics for neutral gas in electron beam ion trap
-
摘要: 在实验室天体物理研究中,电子束离子阱(EBIT)是极端紫外(EUV)和X射线波段能谱分析的重要实验平台,其中EBIT中心残余的中性气体对离子产生存在显著影响。研究了阱区中心残余中性气体对电荷态分布的影响,发现阱区中心残余中性气体和高电荷态离子之间的电荷/能量交换过程不仅影响离子的电荷分布, 而且对激发函数(离子分布比例随电子能量关系曲线)有着极大的影响。利用电离平衡分析方法成功诊断出阱区中心区域残留的中性气体分子数密度,以及内腔室的真空度。Abstract: Electron beam ion traps(EBITs) play an important role on extreme ultra-violet(EUV) and X-ray spectroscopy in laboratory astrophysics. Residual neutral gas in the EBIT trap center has a significant effect on ion breeding. In this work, we investigated the effect of residual neutral gas on the charge state distribution, as well as the diagnostic for the pressure in the trap center. The charge/energy exchange process between the neutral gas and highly charged ions not only affects the ionic fraction, but also plays an important role in fitting the excitation function (namely the relation curve of ionic fraction as a function of electron energies). By using the ionization equilibrium method on the measured excitation function, we have successfully estimated the residual neutral gas in the ion-electron interaction region of the trap center, as well as the vacuum pressure at the trap center.
-
Key words:
- atomic processes /
- electron beam ion trap /
- extreme ultraviolet
-
表 1 实验等离子体中残留气体密度与阱区中心压强
Table 1. Resultant neutral density for the #Fe1008 measurement
ion lg(n0/cm-3) pressure/(10-8 Pa) Fe17+ 6.30±0.56 2.9-2.0+7.5 Fe18+ 6.42±0.64 3.8-2.9+12.3 Fe19+ 6.28±0.60 2.7-2.0+8.2 Fe20+ 6.57±0.64 5.3-4.1+18.0 Fe21+ 6.76±0.56 8.3-6.0+21.7 Fe22+ 6.91±0.66 11.7-9.0+41.7 -
[1] Dere K P, Landi E, Mason H E, et al. CHIANTI—An atomic database for emission lines. Ⅰ. Wavelengths greater than 50 Å[J]. Astronomy and Astrophysics Supplement Series, 1997, 125(1): 149-173. doi: 10.1051/aas:1997368 [2] Landi E, Young P R, Dere K P, et al. CHIANTI—An atomic database for emission lines. ⅩⅢ. Soft X-ray improvements and other changes[J]. The Astrophysical Journal, 2013, 763(2): 86. doi: 10.1088/0004-637X/763/2/86 [3] Smith R K, Brickhouse N S, Liedahl D A, et al. Collisional plasma models with APEC/APED: emission-line diagnostics of hydrogen-like and helium-like ions[J]. The Astrophysical Journal Letters, 2001, 556(2): L91. doi: 10.1086/322992 [4] Foster A R, Ji L, Smith R K, et al. Updated atomic data and calculations for X-ray spectroscopy[J]. The Astrophysical Journal, 2012, 756(2): 128. doi: 10.1088/0004-637X/756/2/128 [5] Smith R K, Foster A R, Brickhouse N S. Approximating the X-ray spectrum emitted from astrophysical charge exchange[J]. Astronomische Nachrichten, 2012, 333(4): 301-304. doi: 10.1002/asna.201211673 [6] Testa P, Drake J J, Landi E. Testing EUV/X-ray atomic data for the solar dynamics observatory[J]. The Astrophysical Journal, 2012, 745(2): 111. doi: 10.1088/0004-637X/745/2/111 [7] Gillaspy J D, Lin T, Tedesco L, et al. Fe XVII X-ray line ratios for accurate astrophysical plasma diagnostics[J]. The Astrophysical Journal, 2011, 728(2): 132. doi: 10.1088/0004-637X/728/2/132 [8] Bernitt S, Brown G V, Rudolph J K, et al. An unexpectedly low oscillator strength as the origin of the Fe XVII emission problem[J]. Nature, 2012, 492(7428): 225. doi: 10.1038/nature11627 [9] Loch S D, Ballance C P, Li Y, et al. Non-equilibrium modeling of the Fe XVII 3C/3D line ratio in an intense X-ray free-electron laser excited plasma[J]. The Astrophysical Journal Letters, 2015, 801(1): L13. doi: 10.1088/2041-8205/801/1/L13 [10] Liang G Y, Baumann T M, López-Urrutia J R C, et al. Extreme-ultraviolet spectroscopy of Fe Ⅵ-Fe ⅩⅤ and its diagnostic application for electron beam ion trap plasmas[J]. The Astrophysical Journal, 2009, 696(2): 2275. doi: 10.1088/0004-637X/696/2/2275 [11] Liang G Y, López-Urrutia J R C, Baumann T M, et al. Experimental investigations of ion charge distributions, effective electron densities, and electron-ion cloud overlap in electron beam ion trap plasma using extreme-ultraviolet spectroscopy[J]. The Astrophysical Journal, 2009, 702(2): 838. doi: 10.1088/0004-637X/702/2/838 [12] Gillaspy J D. Precision spectroscopy of trapped highly charged heavy elements: pushing the limits of theory and experiment[J]. Physica Scripta, 2014, 89: 114004. doi: 10.1088/0031-8949/89/11/114004 [13] Liang G Y, Li F, Wang F L, et al. X-ray and EUV spectroscopy of various astrophysical and laboratory plasmas: Collisional, photoionization and charge-exchange plasmas[J]. The Astrophysical Journal, 2014, 783(2): 124. doi: 10.1088/0004-637X/783/2/124 [14] Hahn M, Becker A, Bernhardt D, et al. Storage ring cross section measurements for electron impact single and double ionization of Fe13+ and single ionization of Fe16+ and Fe17+[J]. The Astrophysical Journal, 2013, 767(1): 47. doi: 10.1088/0004-637X/767/1/47 [15] Dere K P. Ionization rate coefficients for the elements hydrogen through zinc[J]. Astronomy & Astrophysics, 2007, 466(2): 771-792. [16] Kim Y S, Pratt R H. Direct radiative recombination of electrons with atomic ions: Cross sections and rate coefficients[J]. Physical Review A, 1983, 27(6): 2913. doi: 10.1103/PhysRevA.27.2913 [17] Epp S W, López-Urrutia J R C, Brenner G, et al. Soft X-ray laser spectroscopy on trapped highly charged ions at FLASH[J]. Physical review letters, 2007, 98(18): 183001. doi: 10.1103/PhysRevLett.98.183001