Breit-Pauli energy levels and transition rates for nitrogen-like and oxygen-like sequences

89Citations
Citations of this article
19Readers
Mendeley users who have this article in their library.

Abstract

Breit-Pauli results for energy levels, lifetimes, and Landé gJ factors have been determined for all levels up to 2p23d of the nitrogen-like sequence (Z = 7-17) and 2p33d of the oxygen-like sequence (Z = 8-20). Exceptions are some lower members of the sequence where the spectrum included only those levels below the second 2p24s term in the case of N-like or 2p34s in the case of O-like. The computed energy and E1, E2, M1, M2 transition data between all levels, including convergence of the LS line strength for both length and velocity forms, may be viewed at a website. In this paper, critically evaluated transition data is presented for N I, O II, Mg VI, and Si VIII (N-like sequence) and O I, Ne III, Mg V, and Si VII (O-like) for E1 transitions including uncertainty estimates. The accuracy of energy levels is determined by comparison with experiment. Transition rates with uncertainties are compared with experiment and other theory.

Author supplied keywords

Cite

CITATION STYLE

APA

Tachiev, G. I., & Fischer, C. F. (2002). Breit-Pauli energy levels and transition rates for nitrogen-like and oxygen-like sequences. Astronomy and Astrophysics, 385(2), 716–723. https://doi.org/10.1051/0004-6361:20011816

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free