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Phys. Rev. A 74, 042514 (2006) [6 pages]

Accurate modeling of benchmark x-ray spectra from highly charged ions of tungsten

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Yuri Ralchenko*, Joseph N. Tan, J. D. Gillaspy, and Joshua M. Pomeroy
Atomic Physics Division, National Institute of Standards and Technology, Gaithersburg, Maryland 20899-8422, USA

Eric Silver
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, Massachusetts 02138, USA

Received 31 August 2006; published 26 October 2006

We present detailed collisional-radiative modeling for a benchmark x-ray spectrum of highly charged tungsten ions in the range between 3 and 10 Å produced in an electron beam ion trap (EBIT) with a beam energy of 4.08 keV. Remarkably good agreement between calculated and measured spectra was obtained without adjustable parameters, highlighting the well-controlled experimental conditions and the sophistication of the kinetic simulation of the non-Maxwellian tungsten plasma. This agreement permitted the identification of spectral lines from Cu-like W45+ and Ni-like W46+ ions, led to the reinterpretation of a previously known line in Ni-like ion as an overlap of electric-quadrupole and magnetic-octupole lines, and revealed subtle features in the x-ray spectrum arising from the dominance of forbidden transitions between excited states. The importance of level population mechanisms specific to the EBIT plasma is discussed as well.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevA.74.042514
DOI:
10.1103/PhysRevA.74.042514
PACS:
32.30.Rj, 39.10.+j, 52.59.−f

*Electronic address: yuri.ralchenko@nist.gov