Dataset for Optical Processes in Dense Astrophysical and Laboratory Plasmas

The interest in the modeling of laboratory and astrophysical plasma behavior from mid up to strong non-ideality (NI), e.g., plasma in which a Coulomb interaction becomes dominant, led us to further investigate the optical properties of such systems. An expanded set of results and properties like wav...

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Veröffentlicht in:Atoms 2024-11, Vol.12 (11), p.59
Hauptverfasser: Sakan, Nenad M., Srećković, Vladimir A., Simić, Zoran J., Dechev, Momchil
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Sprache:eng
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Zusammenfassung:The interest in the modeling of laboratory and astrophysical plasma behavior from mid up to strong non-ideality (NI), e.g., plasma in which a Coulomb interaction becomes dominant, led us to further investigate the optical properties of such systems. An expanded set of results and properties like wave functions, dipole matrix elements, etc., for such systems is presented in this submission. The methodologies of our research, as well as the current and future elements of their applications, are explained. In addition to being helpful to other researchers for achieving a variety of goals, the data from this study could be useful the interdisciplinary fields of machine learning, astrochemistry and fusion physics. The dataset is available online at the repository Figshare.
ISSN:2218-2004
2218-2004
DOI:10.3390/atoms12110059