Automodel solutions of Biberman-Holstein equation for stark broadening of spectral lines

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dc.bibliographicCitation.articleNumber43
dc.bibliographicCitation.firstPage43
dc.bibliographicCitation.issue3
dc.bibliographicCitation.journalTitleAtoms
dc.bibliographicCitation.volume6
dc.contributor.authorKukushkin, Alexander B.
dc.contributor.authorNeverov, Vladislav S.
dc.contributor.authorSdvizhenskii, Petr A.
dc.contributor.authorVoloshinov, Vladimir V.
dc.date.accessioned2025-02-26T09:42:04Z
dc.date.available2025-02-26T09:42:04Z
dc.date.issued2018
dc.description.abstractThe accuracy of approximate automodel solutions for the Green's function of the Biberman-Holstein equation for the Stark broadening of spectral lines is analyzed using the distributed computing. The high accuracy of automodel solutions in a wide range of parameters of the problem is shown.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/18599
dc.identifier.urihttps://doi.org/10.34657/17618
dc.language.isoeng
dc.publisherBasel : MDPI
dc.relation.doihttps://doi.org/10.3390/atoms6030043
dc.relation.essn2218-2004
dc.rights.licenseCC BY 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/4.0
dc.subject.ddc530
dc.subject.otherAutomodel (self-similar) solutionseng
dc.subject.otherDistributed computingeng
dc.subject.otherStark broadening of spectral lineseng
dc.subject.otherSuperdiffusive transporteng
dc.titleAutomodel solutions of Biberman-Holstein equation for stark broadening of spectral lineseng
dc.typeArticle
dc.typeText
tib.accessRightsopenAccess
wgl.contributorINP
wgl.subjectPhysikger
wgl.typeZeitschriftenartikelger
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