Research Article

Comparison of models for evolution of X-ray satellite lines

  1. T. Mukoyama1,*,
  2. M. Uda2,
  3. L. Kövér3

Article first published online: 22 JUN 2009

DOI: 10.1002/xrs.1194

Issue

X‐Ray Spectrometry

X-Ray Spectrometry

Volume 38, Issue 5, pages 406–409, September/October 2009

Additional Information

How to Cite

Mukoyama, T., Uda, M. and Kövér, L. (2009), Comparison of models for evolution of X-ray satellite lines. X-Ray Spectrometry, 38: 406–409. doi: 10.1002/xrs.1194

Author Information

  1. 1

    Kansai Gaidai University, Hirakata, Osaka 573-1001, Japan

  2. 2

    Waseda University, Doshita 2-40-5, Nerima-ku, Tokyo 179-0086, Japan

  3. 3

    Institute of Nuclear Research of the Hungarian Academy of Sciences (ATOMKI), H-4001 Debrecen, Hungary

*Kansai Gaidai University, Hirakata, Osaka 573-1001, Japan.

Publication History

  1. Issue published online: 25 AUG 2009
  2. Article first published online: 22 JUN 2009
  3. Manuscript Accepted: 5 MAY 2009
  4. Manuscript Received: 26 MAR 2009

Funded by

  • Bilateral Japan-Hungary Cooperative Research Program
  • Hungarian Academy of Sciences. Grant Number: OTKA 67873

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Abstract

Evolution of the KL X-ray satellite line was studied. Four theoretical models based on the adiabatic approximation were fitted to the experimental data for the intensity ratio of the satellite line relative to the diagram line for Fe and Zn as a function of incident photon energy. The Thomas, the Vatai, the Roy and the modified Roy (Roy2) models were considered. Comparison of these four models was made for the case of inner-shell electron transitions and their difference was clarified. The reason that the models developed for bound–bound transitions can give satisfactory results for bound-free transitions is discussed. Copyright © 2009 John Wiley & Sons, Ltd.

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