Electron‐impact excitation of UF6 at an electron energy of 20 eV in the energy‐loss range of 0–10 eV

1976 ◽  
Vol 64 (11) ◽  
pp. 4791-4793 ◽  
Author(s):  
A. Chutjian ◽  
S. K. Srivastava ◽  
S. Trajmar ◽  
W. Williams ◽  
D. C. Cartwright
1991 ◽  
Vol 66 (2) ◽  
pp. 157-160 ◽  
Author(s):  
E. K. Wåhlin ◽  
J. S. Thompson ◽  
G. H. Dunn ◽  
R. A. Phaneuf ◽  
D. C. Gregory ◽  
...  

1991 ◽  
Vol 21 (S1) ◽  
pp. S35-S38
Author(s):  
E. K. W�hlin ◽  
J. S. Thompson ◽  
G. H. Dunn ◽  
R. A. Phaneuf ◽  
D. C. Gregory ◽  
...  

Atoms ◽  
2021 ◽  
Vol 9 (4) ◽  
pp. 76
Author(s):  
Aloka Kumar Sahoo ◽  
Lalita Sharma

In the present work, a detailed study on the electron impact excitation of Xe7+, Xe8+, Xe9+ and Xe10+ ions for the dipole allowed (E1) transitions in the EUV range of 8–19 nm is presented. The multi-configuration Dirac–Fock method is used for the atomic structure calculation including the Breit and QED corrections along with the relativistic configuration interaction approach. We have compared our calculated energy levels, wavelengths and transition rates with other reported experimental and theoretical results. Further, the relativistic distorted wave method is used to calculate the cross sections from the excitation threshold to 3000 eV electron energy. For plasma physics applications, we have reported the fitting parameters of these cross sections using two different formulae for low and high energy ranges. The rate coefficients are also obtained using our calculated cross sections and considering the Maxwellian electron energy distribution function in the electron temperature range from 5 eV to 100 eV.


1996 ◽  
Vol 3 (2) ◽  
pp. 461-467 ◽  
Author(s):  
Peter J. Catto ◽  
Sergei Krasheninnikov ◽  
R. D. Hazeltine

1973 ◽  
Vol 51 (19) ◽  
pp. 2047-2053 ◽  
Author(s):  
John A. Tully

The nonrelativistic Coulomb–Born approximation has been used to compute scaled collision strengths for electron impact excitation of the 1s → ns, np, nd transitions in hydrogenic ions. Results are given for n = 2, 3, 4, 5, 6, [Formula: see text] as a function of the incident electron energy in threshold units. Simple formulae for interpolating the tabulated results are also given.


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