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• W2091225249 abstract "A model is presented where the level-population densities in quasi-steady-state hot dense plasmas are described by means of large nonrelativistic superconfigurations (SC's), whose configuration populations follow a decreasing-exponential law versus energy (Boltzmann like) for a temperature depending on the SC. Two systems of linear equations are obtained. The first one yields the average-state population densities of the SC's. Using these results, the second system yields the SC temperatures. In this model, a very large number of atomic levels is accounted for in a simple way, thus yielding the configuration populations and, hence, the ionic distribution and average charge. It also yields accurate simulations of the spectra, which are of the essence for emissivity and absorption calculations. It opens a way to time-dependent calculations." @default.
• W2091225249 created "2016-06-24" @default.
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• W2091225249 date "2004-02-17" @default.
• W2091225249 modified "2023-10-05" @default.
• W2091225249 title "Model for computing superconfiguration temperatures in nonlocal-thermodynamic-equilibrium hot plasmas" @default.
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• W2091225249 doi "https://doi.org/10.1103/physreve.69.026403" @default.
• W2091225249 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/14995562" @default.
• W2091225249 hasPublicationYear "2004" @default.
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