Published September 2008 | Version v1
Journal article

Fine-structure energy levels, oscillator strengths and lifetimes in Co-XV

  • 1. S. D. (Postgraduate) College, Muzaffarnagar, 251 001, India, affiliated to Chowdhary Charan Singh Univ., Dept. of Physics, Meerut (India)
  • 2. Clark Atlanta Univ., Dept. of Physics and Center for Theoretical Studies of Physical Systems, Atlanta, Georgia (United States)

Description

The study of Al-like spectra of ions of the elements of the iron group has received a great deal of attention because they are of particular interest in controlled thermonuclear fusion. Excitation energies from ground state for 97 fine-structure levels as well as oscillator strengths and radiative decay rates for all electric-dipole-allowed and intercombination transitions among the fine-structure levels of the terms belonging to the (1s22s22p6)3s23p,3s3p2,3s23d, 3p3, 3s3p3d, 3p23d, 3s3d2,3s24s,3s24p,3s24d,3s24f, and 3s3p4s configurations of Co XV 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. Our calculated excitation energies, including their ordering, are in excellent agreement with the experimental results and the experimentally compiled energy values of the National Institute for Standards and Technology (NIST) wherever available. The mixing among several fine-structure levels is found to be very strong, with most of the strongly mixed levels belonging to the (1s22s22p6)3p23d and 3s3d2 configurations. The strong mixing among several fine-structure levels makes it very difficult to identify them uniquely. Perhaps, that may be the reason for the lack of both experimental and theoretical results for these levels. We believe that our extensive calculated values can guide experimentalists in identifying the fine-structure levels in their future work. From our radiative decay rates we have also calculated radiative lifetimes of some fine-structure levels. In this calculation we also predict new data for several fine-structure levels where no other theoretical and/or experimental results are available. (authors)

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Additional details

Identifiers

Publishing Information

Journal Title
European Physical Journal. D, Atomic, Molecular and Optical Physics
Journal Volume
49
Journal Issue
no.2
Journal Page Range
p. 157-160
ISSN
1434-6060

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
40029309
Subject category
S74: ATOMIC AND MOLECULAR PHYSICS;
Descriptors DEI
COBALT IONS; ELECTRONIC STRUCTURE; ENERGY LEVELS; FINE STRUCTURE; LIFETIME; OSCILLATOR STRENGTHS
Descriptors DEC
CHARGED PARTICLES; IONS

Optional Information

Notes
32 refs.