Phys. Rev. A 75, 066501 (2007) [2 pages]Comment on “Direct observation of the 2D3∕2–2D5∕2 ground-state splitting in Xe9+”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
See AlsoOriginal Article: E. Takács, B. Blagojevic, K. Makónyi, E.-O. Le Bigot, C. I. Szabó, Y.-K. Kim, and J. D. Gillaspy, Direct observation of the 2D3∕2-2D5∕2 ground-state splitting in Xe9+, Phys. Rev. A 73, 052505 (2006). |
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