Comparison of second-order spectral line widths formulae

IF 1.6 3区 物理与天体物理 Q3 PHYSICS, FLUIDS & PLASMAS High Energy Density Physics Pub Date : 2024-01-18 DOI:10.1016/j.hedp.2024.101080
Carlos A. Iglesias , Thomas A. Gomez
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Abstract

Frequently used second-order spectral line width formulae from the projector operator and kinetic theory methods have not been formally compared previously. It is shown that a systematic second-order expansion of the projection operator expression including initial correlations agrees with the second-order kinetic theory result. The agreement assumes a common approximation in the projector operator method that introduces a screened radiator–perturber interaction to account for neglected electron–electron correlations. On the other hand, it is shown that the usual width expression from the projection operator approach neglecting initial correlations differs from kinetic theory. The differences, however, are at least third order in the radiator–perturber interaction. The comparisons suggest using the more compact width expression from kinetic theory, which includes initial correlations and a systematic screening of the radiator–perturber interactions, as the starting point for second-order width calculations.

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二阶光谱线宽公式的比较
投影算子和动力学理论方法中常用的二阶光谱线宽公式以前从未正式比较过。研究表明,包括初始相关性在内的投影算子表达式的系统二阶展开与二阶动力学理论结果一致。这种吻合假定了投影算子方法中的一个共同近似值,即引入了屏蔽辐射器-珀特尔相互作用,以解释被忽视的电子-电子相关性。另一方面,研究表明,忽略初始相关性的投影算子法的通常宽度表达式与动力学理论不同。然而,在辐射器-珀特伯相互作用中,这种差异至少是三阶的。比较结果表明,使用动力学理论中更紧凑的宽度表达式作为二阶宽度计算的起点,该表达式包括初始相关性和辐射器-珀特伯相互作用的系统筛选。
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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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