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arXiv 0704.0905astro-ph
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Fe XV形成Fe XIV的双电子取代:实验室测量和理论计算

Dielectronic Recombination of Fe XV forming Fe XIV: Laboratory Measurements and Theoretical Calculations

D. V. Lukić, M. Schnell, D. W. Savin, C. Brandau, E. W. Schmidt, S. Böhm, A. Müller, S. Schippers, M. Lestinsky, F. Sprenger, A. Wolf, Z. Altun, N. R. Badnell

摘要:

在电子-离子碰撞能量0-45 eV范围内,我们测量了类Mg Fe XV通过N=3 -> N' = 3芯激发形成类Al Fe XIV的双电子复合(DR)的共振强度和能量。所有测量都是使用德国海德堡马克斯普朗克核物理研究所的重离子测试储存环进行的。我们还进行了新的多组态Breit-Pauli(MCBP)计算使用AUTOSTRUCTURE代码。对于< 25 eV的电子-离子碰撞能量,我们发现我们的实验和理论共振能量和强度之间的一致性较差。从25到42 eV,我们发现两者之间的共振能量很好的协议。但在这个能量范围内,理论共振强度比实验结果大~ 31%。这比我们在该能量范围内估计的总实验不确定度+/- 26%(置信水平为90%)要大。在42 eV以上,计算的3s 3 p(^1P_1)nl DR系列极限和测量的3s 3 p(^1P_1)nl DR系列极限之间的形状差异部分归因于实验中高里德堡态的探测概率的nl依赖性。我们已经使用我们的测量,辅以我们的AUTOSTRUCTURE计算,以产生Fe XV形成Fe XIV的麦克斯韦平均3 -> 3 DR速率系数。对于k_BT_e > 1 eV,估计所得速率系数的准确度优于+/-29%(在90%置信水平下)。在kBT_e ~ 2.5-15 eV的温度范围内,我们的实验结果与先前发表的理论结果有很大的差异。在此温度范围内,我们新的MCBP血浆速率系数比我们的实验结果小19-28%。

英文摘要:

We have measured resonance strengths and energies for dielectronic recombination (DR) of Mg-like Fe XV forming Al-like Fe XIV via N=3 -> N' = 3 core excitations in the electron-ion collision energy range 0-45 eV. All measurements were carried out using the heavy-ion Test Storage Ring at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We have also carried out new multiconfiguration Breit-Pauli (MCBP) calculations using the AUTOSTRUCTURE code. For electron-ion collision energies < 25 eV we find poor agreement between our experimental and theoretical resonance energies and strengths. From 25 to 42 eV we find good agreement between the two for resonance energies. But in this energy range the theoretical resonance strengths are ~ 31% larger than the experimental results. This is larger than our estimated total experimental uncertainty in this energy range of +/- 26% (at a 90% confidence level). Above 42 eV the difference in the shape between the calculated and measured 3s3p(^1P_1)nl DR series limit we attribute partly to the nl dependence of the detection probabilities of high Rydberg states in the experiment. We have used our measurements, supplemented by our AUTOSTRUCTURE calculations, to produce a Maxwellian-averaged 3 -> 3 DR rate coefficient for Fe XV forming Fe XIV. The resulting rate coefficient is estimated to be accurate to better than +/- 29% (at a 90% confidence level) for k_BT_e > 1 eV. At temperatures of k_BT_e ~ 2.5-15 eV, where Fe XV is predicted to form in photoionized plasmas, significant discrepancies are found between our experimentally-derived rate coefficient and previously published theoretical results. Our new MCBP plasma rate coefficient is 19-28% smaller than our experimental results over this temperature range.

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