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Journal of the Korean Physical Society

, Volume 64, Issue 5, pp 659–666 | Cite as

Theoretical photoionization spectra for the Mg-like S4+ Ion in the energy range between the S5+ 4s and 4f thresholds

  • Dae-Soung KimEmail author
  • Duck-Hee Kwon
Article

Abstract

The partial and the total photoionization cross sections of the Mg-like S4+ ion, leaving the residual S5+ 3l and 4l states from the ground 3s 2 1 S e and the excited 3s3p 3,1 P o initial states, have been calculated for photon energies ranging from the S5+ 4s to the S5+ 4f threshold. The complex features appearing in the cross sections represent the tangled autoionizing Rydberg resonances converging to the different S5+ 4l thresholds. The present results are compared with the available previous National Institute of Standards and Technology(NIST) and Opacity Project(OP) results.

Keywords

Atomic data Atomic process Photoionization Photoelectron Rydberg series Autoionization 

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References

  1. [1]
    G. N. Bates and P. L. Altic, J. Phys. B 6, 653 (1973).ADSCrossRefGoogle Scholar
  2. [2]
    J. Dubau and J. Wells, J. Phys. B 6, L31 (1973).ADSCrossRefGoogle Scholar
  3. [3]
    C. H. Greene, Phys. Rev. A 23, 661 (1981).ADSCrossRefGoogle Scholar
  4. [4]
    P. F. O’Mahony and C. H. Greene, Phys. Rev. A 31, 250 (1985).ADSCrossRefGoogle Scholar
  5. [5]
    V. Radojevic and W. R. Johnson, Phys. Rev. A 31, 2991 (1985).ADSCrossRefGoogle Scholar
  6. [6]
    R. Moccia and P. Spizzo, J. Phys. B 21, 1133 (1988).ADSCrossRefGoogle Scholar
  7. [7]
    Z. Altun, Phys. Rev. A 40, 4968 (1989).ADSCrossRefGoogle Scholar
  8. [8]
    K. Butler, C. Mendoza and C. J. Zeippen, Mon. Not. R. Astr. Soc. 209, 343 (1984).ADSGoogle Scholar
  9. [9]
    K. Butler, C. Mendoza and C. J. Zeippen, Mon. Not. R. Astr. Soc. 213, 345 (1985).ADSGoogle Scholar
  10. [10]
    K. Butler, C. Mendoza and C. J. Zeippen, J. Phys. B 26, 4409 (1993).ADSCrossRefGoogle Scholar
  11. [11]
    H.-C. Chi and K.-N. Huang, Phys. Rev. A 50, 392 (1994).ADSCrossRefGoogle Scholar
  12. [12]
    H.-C. Chi, Phys. Rev. A 56, 4118 (1997).ADSCrossRefGoogle Scholar
  13. [13]
    D.-S. Kim and S. S. Tayal, J. Phys. B 33, 3235 (2000).ADSCrossRefGoogle Scholar
  14. [14]
    D.-S. Kim, J. Phys. B 34, 2615 (2001).ADSCrossRefGoogle Scholar
  15. [15]
    D.-S. Kim and Y. S. Kim, J. Phys. Soc. Jpn. 76, 014302 (2007).ADSCrossRefGoogle Scholar
  16. [16]
    D.-S. Kim and Y. S. Kim, J. Phys. B 41, 165002 (2008).ADSCrossRefGoogle Scholar
  17. [17]
    D.-S. Kim and F. Koike, J. Phys. Soc. Jpn. 77, 124302 (2008).ADSCrossRefGoogle Scholar
  18. [18]
    D.-S. Kim and D.-H. Kwon, Phys. Rev. A 88, 033426 (2013).ADSCrossRefGoogle Scholar
  19. [19]
    M. Seaton, J. Phys. B 20, 6363 (1987).ADSCrossRefGoogle Scholar
  20. [20]
    OP Team, The Opacity Project, Vol. 1 (Institute of Physics Publishing, Briston, UK, 1995).Google Scholar
  21. [21]
  22. [22]
    G. Mehlman-Balloffet and J. M. Esteva, Astrophys. J. 157, 945 (1969).ADSCrossRefGoogle Scholar
  23. [23]
    J. M. Preses, C. E. Burkhardt, W. P. Garver and J. J. Leventhal, Phys. Rev. A 29, R985 (1984).ADSCrossRefGoogle Scholar
  24. [24]
    W. Fiedler, C. Kortenkamp and P. Zimmermann, Phys. Rev. A 36, 384 (1987).ADSCrossRefGoogle Scholar
  25. [25]
    G. W. Schinn, C. J. Dai and T. F. Gallagher, Phys. Rev. A 43, 2316 (1991).ADSCrossRefGoogle Scholar
  26. [26]
    R. Wehlitz, D. Lukić and P. N. Juranić, J. Phys. B 40, 2385 (2007).ADSCrossRefGoogle Scholar
  27. [27]
    J. B. West, T. Andersen, R. L. Brooks, F. Folkmann, H. Kjeldsen and H. Knudsen, Phys. Rev. A 63, 052719 (2001).ADSCrossRefGoogle Scholar
  28. [28]
    M. H. Sayyad, E. T. Kennedy, L. Kiernan, J.-P. Mosnier and J. T. Costello, J. Phys. B 28, 1715 (1995).ADSCrossRefGoogle Scholar
  29. [29]
    A. L. Broadfoot, B. R. Sandel, D. E. Shamansky, J. C. McConnell, G. R. Smith, J. B. Holberg, S. K. Atreya, T. M. Donahue, D. F. Strobel and J. L. Bertaux, Geophys. Res. 86, 8259 (1981).ADSCrossRefGoogle Scholar
  30. [30]
    D. E. Shamansky and G. R. Smith, Geophys. Res. 86, 9179 (1981).ADSCrossRefGoogle Scholar
  31. [31]
    F. Robicheaux, Phys. Rev. A 43, 5946 (1991).ADSCrossRefGoogle Scholar
  32. [32]
    C. H. Greene and C. Jungen, Adv. At. Mol. Phys. 21, 51 (1985).ADSCrossRefGoogle Scholar
  33. [33]

Copyright information

© The Korean Physical Society 2014

Authors and Affiliations

  1. 1.Department of mechanical automationGyeonggi College of Science and TechnologySiheungKorea
  2. 2.Nuclear Data CenterKorea Atomic Energy Research InstituteDaejeonKorea

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