qcx#h0_en2_kvi#ne10.dat

Charge Exchange Cross Sections

Ion
Ne10+
Energy Range
0.010 keV/amu → 100 keV/amu

ADF01

Filename
qcx#h0_en2_kvi#ne10.dat
Full Path
adf01/qcx#h0/qcx#h0_en2_kvi#ne10.dat
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Ne10+ + H0(n=2) → Ne9+ + H+total
Ne10+ + H0(n=2) → Ne9+(n=6) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(6s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(6p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(6d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(6f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(6g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(6h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=7) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(7s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(7i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=8) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(8s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(8j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=9) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(9s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(9k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=10) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(10s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(10l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=11) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(11s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(11m) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=12) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(12s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12m) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(12n) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=13) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(13s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13m) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13n) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(13o) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=14) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(14s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14m) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14n) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14o) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(14q) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(n=15) + H+n-resolved
Ne10+ + H0(n=2) → Ne9+(15s) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15p) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15d) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15f) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15g) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15h) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15i) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15j) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15k) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15l) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15m) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15n) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15o) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15q) + H+nl-resolved
Ne10+ + H0(n=2) → Ne9+(15r) + H+nl-resolved
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  Source:  The data consists of results of CTMC calculations made at the University of Missouri over 
              the period 1995-97.
     
  Comments:  At this time, no direct comparison with other results is available for checking the 
             quality of the nl selective cross-sections except for Li+3 for which results are given
             in a recent hidden curve crossing calculation by Janev et al. (1996).  Large differences
             are observed in both the magnitude and energy dependence.  From inspection of the total
             cross-sections, we have the strong impression that the CTMC data should be preferred.
             In a plot of the scaled total one-electron capture cross-sections (sigma_tot(16q)^-1)
             versus scaled energy (4Eq^-1/2), the total cross-sections should be approximately the
             same for all systems (Janev, 1991) at least for q>3.  In these scaled units, a 
             recommendation by Janev and Smith (1995) has been presented.  The CTMC data are all close 
             to this curve except at lower energies.  The hidden curve crossing data for Li+3 deviate
             from this curve.  Molecular orbital calculations by Errea et al. (1996) for B+5 are in
             good agreement with the corresponding CTMC data.  For He+2, the recommendation of Janev
             and Smith is based on the calculations of Harel and Jouin (1990) and it is completely
             different from the CTMC results for He+2, especially at the lower energies.  A reason
             for this huge difference is hard to see.  It may be the extremely strong resonant 
             nature of the electron capture at low collision energies.  Resonant transfer from H(n=2)
             in collsions with He+2 would necessarily mean that the electron ends up exactly between
             the n=3 and n=4 levels of He+1.  Therefore electron capture may be blocked. To what extent
             this is well described by the CTMC method is still a point of discussion.  For higher
             charged receiver ions, levels are resonantly present.  Except for He+2 at low energies, 
             we recommend use of the present CTMC data. 

             The data was assembled as ADAS data files of type adf01 at JET Joint Undertaking in the
             period 22-23 Dec. 1997.    

  Authors:   J. W. Turkstra, G. Lubinski, R. Hoekstra*, R. E. Olson#
                  * KVI, Groningen, Netherlands
                  # University of Missouri, Rolla, USA. 

  Date:  23 December 1997.

  Updates: 

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