Second-order spectral line shift comparisons

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS
Carlos A. Iglesias , Thomas A. Gomez
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引用次数: 0

Abstract

The second-order spectral line width formulae from the projection operator and kinetic theory methods were recently compared. It was shown that a systematic expansion of the projection operator width expression including initial correlations formally agrees with the second-order kinetic theory result. It is now shown that the second-order dynamic shifts are also formally the same. The static shifts, however, differ due to an ad hoc treatment of electron-electron correlations in the projection operator method. The approximation is necessary in order to screen the radiator-electron interactions. The differences, however, are expected to be small. The results suggest using the rigorous and more compact second-order width and shift expressions from the kinetic theory method as the starting point for spectral line shape calculations. At line center, however, the projection operator second-order expression for the width and shift simplifies and reduces to the kinetic theory result.

二阶谱线偏移比较
最近对投影算子和动力学理论方法得出的二阶光谱线宽公式进行了比较。结果表明,投影算子宽度表达式的系统扩展(包括初始相关性)与二阶动力学理论结果在形式上是一致的。现在的研究表明,二阶动态偏移在形式上也是相同的。然而,由于投影算子方法中对电子-电子相关的特别处理,静态偏移有所不同。为了屏蔽辐射器-电子间的相互作用,这种近似是必要的。不过,差异预计很小。结果表明,使用动力学理论方法中更严谨、更紧凑的二阶宽度和位移表达式作为光谱线形计算的起点。然而,在谱线中心,投影算子二阶宽度和位移表达式简化并还原为动力学理论结果。
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来源期刊
High Energy Density Physics
High Energy Density Physics PHYSICS, FLUIDS & PLASMAS-
CiteScore
4.20
自引率
6.20%
发文量
13
审稿时长
6-12 weeks
期刊介绍: High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings. Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.
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