Published November 2010
| Version v1
Journal article
Experimental and theoretical lifetimes and transition probabilities in Sb i
Creators
- 1. Astrophysique et Spectroscopie, Universite de Mons-UMONS, Place du Parc, 20, B-7000 Mons (Belgium)
- 2. Department of Physics, Lund University, Box 118, SE-221 00 Lund (Sweden)
- 3. Department of Astronomy and Theoretical Physics, Lund University, Box 43, SE-221 00 Lund (Sweden)
Description
We present experimental atomic lifetimes for 12 levels in Sb i. The levels belong to the 5p2(3P)6s 2P, 4P, and 5p2(3P)5d 4P, 4F, and 2F terms. The lifetimes were measured using time-resolved laser-induced fluorescence. In addition, we report calculations of transition probabilities in Sb i using a multiconfigurational Dirac-Hartree-Fock method. The physical model was tested through comparisons between theoretical and experimental lifetimes for 5d and 6s levels. The lifetimes of the 5d 4F3/2,5/2,7/2 levels (19.5, 7.8, and 54 ns, respectively) depend strongly on the J value. This is explained by different degrees of level mixing for the different levels in the 4F term.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevA.82.052512;
- arXiv
- arXiv:1012.4285v1;
Publishing Information
- Journal Title
- Physical Review. A
- Journal Volume
- 82
- Journal Issue
- 5
- Journal Page Range
- p. 052512-052512.8
- ISSN
- 1050-2947
- CODEN
- PLRAAN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43008470
- Subject category
- S74: ATOMIC AND MOLECULAR PHYSICS;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- ANTIMONY; COMPARATIVE EVALUATIONS; ENERGY LEVELS; EXPERIMENTAL DATA; FLUORESCENCE; HARTREE-FOCK METHOD; LIFETIME; PROBABILITY; THEORETICAL DATA; TIME RESOLUTION
- Descriptors DEC
- APPROXIMATIONS; CALCULATION METHODS; DATA; ELEMENTS; EMISSION; EVALUATION; INFORMATION; LUMINESCENCE; METALS; NUMERICAL DATA; PHOTON EMISSION; RESOLUTION; TIMING PROPERTIES
Optional Information
- Notes
- (c) 2010 The American Physical Society