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Phys. Rev. A 75, 066501 (2007) [2 pages]

Comment on “Direct observation of the 2D3/2–2D5/2 ground-state splitting in Xe9+”

C. Biedermann and R. Radtke
AG Plasmaphysik, Institut für Physik der Humboldt-Universität zu Berlin, Newtonstrasse 15, 12489 Berlin, Germany and Max-Planck-Institut für Plasmaphysik, EURATOM Association, Greifswald, Germany
Received 2 February 2007; published 15 June 2007

We have found that xenon in different charge states, namely, Xe9+ and Xe31+, can contribute to the radiation in the 598  nm spectral range. Our observation resolves the discrepancy of line identification given by Takács et al. [Phys. Rev. A 73, 052505 (2006)] and Crespo et al. [Can. J. Phys. 80, 1687 (2002)].

©2007 The American Physical Society

URL: http://link.aps.org/doi/10.1103/PhysRevA.75.066501
DOI: 10.1103/PhysRevA.75.066501
PACS: 32.30.Jc; 31.15.Ar; 85.40.Hp; 31.30.Jv
  • 32.30.Jc
    Visible and ultraviolet atomic spectra
  • 31.15.Ar
    Ab initio calculations (atoms and molecules)
  • 85.40.Hp
    Lithography, masks and pattern transfer (microelectronics)
  • 31.30.Jv
    Relativistic and quantum electrodynamic effects in atoms and molecules
  • YEAR: 2007
KEYWORDS: xenon, ground states, visible spectra

See Also

Direct observation of the 2D3/2-2D5/2 ground-state splitting in Xe9+
E. Takács, B. Blagojevic, K. Makónyi et al.
Phys. Rev. A 73, 052505 (2006)

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Related Articles

  1. Direct observation of the 2D3/2-2D5/2 ground-state splitting in Xe9+
    E. Takács, B. Blagojevic, K. Makónyi et al.
    Phys. Rev. A 73, 052505 (2006)


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