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Radiative decay from the 7s1/2 level in Pb+ and transition probabilities of astrophysical interest in Pb+ and Bi++

Author
QUINET, P1 2 ; BIDMONT, E1 2 ; PALMERI, P1 ; XU, H. L3
[1] Astrophysique et Spectroscopie, Université de Mons-Hainaut, 7000 Mons, Belgium
[2] IPNAS, Sart-Tilman B15, Université de Liège, 4000 Liège, Belgium
[3] Department of Physics, Laval University, Québec G1K 7P4, Canada
Source

Journal of physics. B. Atomic, molecular and optical physics (Print). 2007, Vol 40, Num 10, pp 1705-1712, 8 p ; ref : 3/4 p

CODEN
JPAPEH
ISSN
0953-4075
Scientific domain
Atomic molecular physics
Publisher
Institute of Physics, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Keyword (fr)
Approximation multiconfigurationnelle Bismuth Ion atomique Durée vie radiative Durée vie Etude théorique Fluorescence induite par laser Ion multichargé Molécule interstellaire Probabilité transition Théorie Dirac Fock 3270C Bi ip 2 Pb ip 1 Plomb Ion atomique
Keyword (en)
Multiconfiguration approximation Bismuth Atomic ions Radiative lifetimes Lifetime Theoretical study Laser induced fluorescence Multicharged ions Interstellar molecules Transition probabilities Dirac-Fock theory
Keyword (es)
Aproximación multiconfiguracional
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B30 Atomic and molecular physics / 001B30B Atomic properties and interactions with photons / 001B30B70 Intensities and shapes of atomic spectral lines / 001B30B70C Oscillator strengths, lifetimes, transition moments

Discipline
Atomic and molecular physics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18768060

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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