[Ni I] & [Ni II] transition probabilities (Quinet+, 1996)

Physics – Atomic Physics

Scientific paper

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Atomic Physics

Scientific paper

New radiative transition probabilities have been calculated for forbidden lines of astrophysical interest in Ni I and Ni II. The accuracy of the transition probability scales is established on the basis of two independent calculations performed with the approximately relativistic Hartree-Fock (HFR) and SUPERSTRUCTURE (SST) codes. Both physical models take into account the most important configuration interaction (CI) and relativistic effects. (2 data files).

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