Energy Levels, Lifetimes, and Transition Properties for N iii – v
We present excitation energies, transition wavelengths, electric dipole (E1) transition rates, oscillator strengths, line strengths, and lifetimes for the 86 lowest states up to and including 1s22s27f in N iii, the 125 lowest states up to and including 1s22s7f in N iv, and the 53 lowest states up to 1s28g in N v using the multiconfiguration Dirac–Hartree–Fock (MCDHF) and relativistic configuration interaction (RCI) methods. The computed results are then compared with data from the Atomic Spectra Database of the National Institute of Standards and Technology (NIST-ASD), experimental results, and other theoretical studies. For all levels in N iii – v, the root mean square energy differences from the NIST values are 130, 103, and 6 cm−1, respectively. Compared to previous multiconfiguration Hartree–Fock and the Breit–Pauli (MCHF-BP) calculations, 89.3%, 98.5%, and 100% of the log(gf) values for N iii – v agree within 5%, respectively.
Authors
- Kaijian Huang (ORCID: https://orcid.org/0000-0002-4824-0455)
- Juan Du (ORCID: https://orcid.org/0000-0003-2077-3337)
- Meichun Li
- Wenxian Li
Institutions
- Chinese Academy of Sciences (CN)
- National Astronomical Observatories (CN)
- Huizhou University (CN)
Publication Details
- Journal
- Atoms
- Published
- 2025-06-06
- DOI
- https://doi.org/10.3390/atoms13060049
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- National Natural Science Foundation of China
- National Key Research and Development Program of China
- Basic and Applied Basic Research Foundation of Guangdong Province