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• W1978514519 abstract "Theoretical binding energies have been obtained for the metastable ${mathrm{np}}^{3}{}^{4}{S}^{o}$ states in the alkaline-earth sequence using a B-spline configuration-interaction approach. The results agree with available experimental and theoretical data within 5 meV for ${mathrm{Be}}^{ensuremath{-}}$ and within 10 meV for ${mathrm{Mg}}^{ensuremath{-}}.$ The binding energies of the ${p}^{3}{}^{4}{S}^{o}$ state in ${mathrm{Mg}}^{ensuremath{-}},$ ${mathrm{Ca}}^{ensuremath{-}},$ and ${mathrm{Sr}}^{ensuremath{-}}$ are larger than the one in ${mathrm{Be}}^{ensuremath{-}}$ by roughly 250 meV due to the stronger interactions with the ${d}^{2}p$ configurations. For ${mathrm{Ca}}^{ensuremath{-}},$ the ${}^{4}{S}^{o}$ binding energy is determined to be 555.5 meV, including a contribution of $ensuremath{-}70$ meV due to dielectronic core polarization. For ${mathrm{Sr}}^{ensuremath{-}}$ the ${}^{4}{S}^{o}$ binding energy is 557.9 meV, including a decrease of only 6 meV due to dielectronic core polarization. This behavior for the ${}^{4}{S}^{o}$ states in ${mathrm{Ca}}^{ensuremath{-}}$ and ${mathrm{Sr}}^{ensuremath{-}}$ is ascribed to the different neutral-atom states to which the ${}^{4}{S}^{o}$ states are bound." @default.
• W1978514519 created "2016-06-24" @default.
• W1978514519 creator A5038870910 @default.
• W1978514519 date "1999-02-01" @default.
• W1978514519 modified "2023-09-27" @default.
• W1978514519 title "Energies of metastable4Sostates in the alkaline-earth sequence" @default.
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• W1978514519 doi "https://doi.org/10.1103/physreva.59.1125" @default.
• W1978514519 hasPublicationYear "1999" @default.
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