E1 transitions between states with n = 1 to 6 in helium-like carbon, nitrogen, oxygen, neon, silicon, and argon

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dc.creatorJohnson, W. R.
dc.creatorSavukov, I. M.
dc.creatorSafronova, U. I.
dc.creatorDalgarno, A.
dc.date2002-01-28
dc.date2002-02-13
dc.date.accessioned2026-07-07T10:31:11Z
dc.date.available2026-07-07T10:31:11Z
dc.descriptionWavelengths and transition rates are given for E1 transitions between singlet S, P, D, and F states, between triplet S, P, and D states, and between triplet P and singlet S states in ions of astrophysical interest: helium-like carbon, nitrogen, oxygen, neon, silicon, and argon. All possible E1 transitions between states with J < 4 and n < 7 are considered. Energy levels and wave functions used in calculations of the transition rates are obtained from relativistic configuration-interaction calculations that include both Coulomb and Breit interactions.
dc.descriptionsubmitted to Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0201454
dc.identifierhttp://arxiv.org/abs/astro-ph/0201454
dc.identifierAstrophys.J.Suppl.141:543,2002
dc.identifierdoi:10.1086/340547
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178326
dc.subjectAstrophysics
dc.titleE1 transitions between states with n = 1 to 6 in helium-like carbon, nitrogen, oxygen, neon, silicon, and argon
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