Correlation effects are shown to change generalized oscillator strengths and inelr&c form factors by large factors a5 large as 10, from the Hartree-Fock values. The effects are fully included in the charge wavefunctions of the non-closed shell mny-electron theory by Sirmna~u. We calculate ihe charge
Relativistic energies of 1s2, 1s22s and 1s22s2 isoelectronic sequences in first- and second-row atoms
✍ Scribed by Gövel Erol; Iskender Öksüz
- Publisher
- Elsevier Science
- Year
- 1973
- Tongue
- English
- Weight
- 331 KB
- Volume
- 19
- Category
- Article
- ISSN
- 0009-2614
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✦ Synopsis
An acxuate semi-empirical method based on the many-ekctron theory of Sinano@u for calcukting relativistic contributions to atomic energies is developed and applied to the Is', 1~~2s and ls22s2 isoelectronic seiuences in the fist and second periods. Orbital additivity of relativistic energies is tested and found to be an inaccurate assumption for small Z.
📜 SIMILAR VOLUMES
Radiationless transition rates to L 1 vacancy states have been calculated ab initio in the Dirac-Fock approximation. The calculations include quantum-electrodynamic corrections. Results in the j j coupling scheme for all possible L 1 transitions are tabulated for elements Yb and Hg.
We preses the SI -1 So fluorescente spectrum, between 740 and 940 om, of azulene sohitions (íOm3 M ìn methanol) excited wïth a @svitched ruby laser. The nitrogerrlaser excïted Sz + SI fíuorescence spectrum, between 700 and 930 om, is also reporteb Tbe transient St + Sn s@etrmn between 500 and 6.50 r