M. Wang, M. O. Larsson, A. Arnesen, R. Hallin, F. Heijkenskjöld, C. Nordling, and A. Wännström, "Collision-based spectroscopy of Xe vi Rydberg states," J. Opt. Soc. Am. B 13, 2715-2719 (1996)
The photon emission from 60-keV Xe6+ colliding with Na or Ar was recorded in the 35–800-nm wavelength region. Several of the observed lines were classified as transitions from singly excited states in Xe5+. The dipole polarizability of Xe6+ and the ionization energy of Xe5+ were determined from a fit with the polarization formula to the experimentally determined energy levels of nonpenetrating states. The analysis was assisted by Hartree–Fock calculations. All Xe5+ lines in the range 35–800 nm, reported in this work or previously, are tabulated.
M. Wang, M. O. Larsson, A. Arnesen, R. Hallin, F. Heijkenskjöld, C. Nordling, and A. Wännström, "Collision-based spectroscopy of Xe vi Rydberg states," J. Opt. Soc. Am. B 14, 1515-1515 (1997) https://opg.optica.org/josab/abstract.cfm?uri=josab-14-6-1515
M. Wang, A. Arnesen, R. Hallin, F. Heijkenskjöld, M. O. Larsson, A. Wännström, A. G. Trigueiros, and A. V. Loginov J. Opt. Soc. Am. B 14(12) 3277-3281 (1997)
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The dashes mean that the line was not visible in the spectrum. The results of series i–v are from Larsson et al.1
Observed vacuum wavelengths.
HFR-calculated vacuum wavelengths.
Intensity of lines observed following Xe6+ collisions with Na, Ar, and He. , where σlevels is the transition energy obtained from levels given in Table 3.
References where the wavelengths were obtained.
Table 3
Energy Levels of Xe vi Established in This and in Previous Works
The experimental energies are based on levels given in Table 2.
Comparison with HFR-calculated energies.
HFR calculations. Only percentages larger than 5% are listed. Underlined numbers indicate negative eigenvectors.
References where the energy levels are obtained.
Tables (3)
Table 1
Experimental Conditions and Related Data for the Experimental Series with Xe6+ as Projectile in This Worka
The dashes mean that the line was not visible in the spectrum. The results of series i–v are from Larsson et al.1
Observed vacuum wavelengths.
HFR-calculated vacuum wavelengths.
Intensity of lines observed following Xe6+ collisions with Na, Ar, and He. , where σlevels is the transition energy obtained from levels given in Table 3.
References where the wavelengths were obtained.
Table 3
Energy Levels of Xe vi Established in This and in Previous Works
The experimental energies are based on levels given in Table 2.
Comparison with HFR-calculated energies.
HFR calculations. Only percentages larger than 5% are listed. Underlined numbers indicate negative eigenvectors.
References where the energy levels are obtained.