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Nuclear Physics: A Key Ingredient in Astrophysical Modeling

✍ Scribed by F.-K. Thielemann; D. Argast; F. Brachwitz; J.L. Fisker; C. Fröhlich; R. Hirschi; E. Kolbe; D. Mocelj; T. Rauscher


Publisher
Elsevier Science
Year
2005
Tongue
English
Weight
564 KB
Volume
751
Category
Article
ISSN
0375-9474

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Spectral line shapes modeling in laborat
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An overview of several spectral line shapes studies of common interest in astrophysical and laboratory plasmas is presented. For lines dominated by Stark broadening, approaches taking into account the dynamics of numerous perturbers are sometimes required. We briefly recall ab initio simulation tech