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Eur. Phys. J. D 44, 449-457 (2007)
DOI: 10.1140/epjd/e2007-00217-3
Fine-structure energy levels, oscillator strengths and lifetimes in Mg-like chromium
Vikas Tayal and G.P. GuptaDepartment of Physics, S. D. (Postgraduate) College, Muzaffarnagar (U.P.) (Affiliated to Choudhary Charan Singh University), Meerut (U.P), India
tayalvikas11@rediffmail.com
(Received 27 December 2006 / Received in final form 4 June 2007 / Published online 29 June 2007)
Abstract
Excitation energies from ground state for 86 fine-structure levels as well
as oscillator strengths and radiative decay rates for all fine-structure
transitions among the levels of the terms
(1s22s22p6)3
s2(1S), 3s3p(1,3P
,
3s3d(1,3D), 3s4s(1,3S), 3s4p(1,3P
, 3s4d(1,3D),
3s4f(1,3F
, 3
p2(1S, 3P, 1D),
3p3d(1,3P
, 1,3D
, 1,3F
,
3p4s(1,3P
, 3p4p(1,3S, 1,3P, 1,3D),
3p4d(1,3P
, 1,3D
, 1,3F
, 3p4f(1,3D,
1,3F, 1,3G) and 3
d2(1S, 3P, 1D, 3F,1G) of Cr
XIII are calculated using extensive configuration-interaction
(CI) wave functions obtained with the CIV3 computer code of Hibbert. The
important relativistic effects in intermediate coupling are included through
the Breit-Pauli approximation via spin-orbit, spin-other-orbit, spin-spin,
Darwin and mass correction terms. Small adjustments to the diagonal elements
of the Hamiltonian matrices have been made. The mixing among several
fine-structure levels is found to be very strong. Our excitation energies,
including their ordering, are in excellent agreement (better than 0.5%)
with the available experimental results. From our transition probabilities,
we have also calculated radiative lifetimes of some fine-structure levels.
Our calculated lifetime for the longer-lived level 3s3p(3P1) is
found to be in excellent agreement with the experimental result of Curtis
compared to other theoretical calculations.
32.10.Fn - Fine and hyperfine structure.
32.70.Cs - Oscillator strengths, lifetimes, transition moments.
95.30.Ky - Atomic and molecular data, spectra, and spectral parameters (opacities, rotation constants, line identification, oscillator strengths, gf values, transition probabilities, etc.).
© EDP Sciences, Società Italiana di Fisica, Springer-Verlag 2007
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