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Phys. Rev. A 58, 2920–2925 (1998)

Electron-impact excitation of Co2+

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J. A. Shaw and M. S. Pindzola
Department of Physics, Auburn University, Auburn, Alabama 36849

N. R. Badnell
Department of Physics and Applied Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom

D. C. Griffin
Department of Physics, Rollins College, Winter Park, Florida 32789

Received 1 April 1998; published in the issue dated October 1998

Electron-impact excitation cross sections and Maxwellian-averaged rate coefficients are calculated from the ground 3d74F to the first 3d74P and the second 3d72G excited terms in Co2+ in close coupling with 8 and 27 terms; much larger transition arrays were first explored in a distorted-wave approximation. Both transitions are important elements of the emission spectrum of type Ia supernovae. We find that the two excitations are dominated by autoionizing resonances attached to higher-lying excited terms in the 3d7, 3d64s, 3d64p, and 3d64d configurations. Those LS terms that are strongly excited from the ground 3d74F, as found by distorted-wave calculations, are included in a large R-matrix calculation using asymptotics based on multichannel quantum defect theory.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.58.2920
DOI:
10.1103/PhysRevA.58.2920
PACS:
34.80.Kw