2013
DOI: 10.1007/s00340-013-5586-z
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Measurement of femtosecond atomic lifetimes using ion traps

Elmar Träbert
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Cited by 9 publications
(5 citation statements)
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References 24 publications
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“…These experiments with an uncertainty larger than 0.5% are however not sensitive enough to test the underlying relativistic correlations and the leading QED effects. New experiments with the soft x-ray free electron laser (FLASH) and a new EBIT [41] along with the pump probe x-ray laser experiments [42] are hopeful to provide experimental data for the transitions with short lifetimes in so far inaccessible energy ranges. We believe that our calculations will support such future experiments for transitions with different frequencies and lifetimes.…”
Section: Resultsmentioning
confidence: 99%
“…These experiments with an uncertainty larger than 0.5% are however not sensitive enough to test the underlying relativistic correlations and the leading QED effects. New experiments with the soft x-ray free electron laser (FLASH) and a new EBIT [41] along with the pump probe x-ray laser experiments [42] are hopeful to provide experimental data for the transitions with short lifetimes in so far inaccessible energy ranges. We believe that our calculations will support such future experiments for transitions with different frequencies and lifetimes.…”
Section: Resultsmentioning
confidence: 99%
“…An experiment that was thought to be particularly clean, in an EBIT at the LCLS X-Ray light source, did not cut through the fog either [82], and the astrophysical interpretative struggle continued [83]. An attempt at measuring the two level lifetimes expected from theory (44 fs and 166 fs, respectively) unfortunately failed [84]. Further attempts continued to find the reasons for the line ratio being different from the theory for Ne-like ions, assuming, for example, nonlinear excitation dynamics or population transfers from adjacent charge state ions [85] (for further references, see [86]).…”
Section: Ne-like Fe XVIImentioning
confidence: 99%
“…HCI光谱是 了解天体物质成分、离子所处天体的等离子体环境 状态等关键参数最直接甚至是唯一的手段, 对于理 解和发展天体物理和宇宙模型必不可少 [3] . HCI的 光电离截面、光吸收截面、能级寿命、跃迁速率等 基本参数, 对于研究从太阳日冕到星系中心黑洞周 围的吸积盘等天体物理中等离子体的密度、温度等 特性具有重要意义 [4,5] . 目前对于低价离子的光电 离实验数据和理论模型计算结果符合比较好, 但对 于高价HCI离子, 理论计算与实验测量值偏差较 大, 需要大量高精度的绝对光电离截面测量数据 来验证及修正相关理论模型 [6,7] .…”
Section: 引 言unclassified