Relativistic distortedwave collision strengths for the 16 $\Delta n=0$ optically allowed transitions with $n=2$ in the 67 Olike ions with $26\le Z\le 92$
 Authors:
 Publication Date:
 Sponsoring Org.:
 USDOE
 OSTI Identifier:
 1246483
 Grant/Contract Number:
 AC5206NA25396
 Resource Type:
 Journal Article: Publisher's Accepted Manuscript
 Journal Name:
 Atomic Data and Nuclear Data Tables
 Additional Journal Information:
 Journal Volume: 101; Journal Issue: C; Related Information: CHORUS Timestamp: 20170623 16:10:51; Journal ID: ISSN 0092640X
 Publisher:
 Elsevier
 Country of Publication:
 United States
 Language:
 English
Citation Formats
Fontes, Christopher J., and Zhang, Hong Lin. Relativistic distortedwave collision strengths for the 16 Δ n = 0 optically allowed transitions with n = 2 in the 67 Olike ions with 26 ≤ Z ≤ 92. United States: N. p., 2015.
Web. doi:10.1016/j.adt.2014.08.002.
Fontes, Christopher J., & Zhang, Hong Lin. Relativistic distortedwave collision strengths for the 16 Δ n = 0 optically allowed transitions with n = 2 in the 67 Olike ions with 26 ≤ Z ≤ 92. United States. doi:10.1016/j.adt.2014.08.002.
Fontes, Christopher J., and Zhang, Hong Lin. 2015.
"Relativistic distortedwave collision strengths for the 16 Δ n = 0 optically allowed transitions with n = 2 in the 67 Olike ions with 26 ≤ Z ≤ 92". United States.
doi:10.1016/j.adt.2014.08.002.
@article{osti_1246483,
title = {Relativistic distortedwave collision strengths for the 16 Δ n = 0 optically allowed transitions with n = 2 in the 67 Olike ions with 26 ≤ Z ≤ 92},
author = {Fontes, Christopher J. and Zhang, Hong Lin},
abstractNote = {},
doi = {10.1016/j.adt.2014.08.002},
journal = {Atomic Data and Nuclear Data Tables},
number = C,
volume = 101,
place = {United States},
year = 2015,
month = 1
}
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Relativistic distortedwave collision strengths for the 49 Δn=0 optically allowed transitions with n=2 in the 67 Blike ions with 26≤Z≤92
Relativistic distortedwave collision strengths have been calculated for the 49 Δn=0 optically allowed transitions with n=2 in the 67 Blike ions with nuclear charge number Z in the range 26≤Z≤92. The calculations were made for the four final, or scattered, electron energies E{sup ′}=0.20, 0.42, 0.80, and 1.40, where E{sup ′} is in units of Z{sub eff}{sup 2} Ry with Z{sub eff}=Z−3.33. In the present calculations, an improved “topup” method, which employs relativistic plane waves, was used to obtain the high partialwave contribution for each transition, in contrast to the partialrelativistic Coulomb–Bethe approximation used in previous work by Zhang andmore » 
Relativistic distortedwave collision strengths for the 49 Δn=0 optically allowed transitions with n=2 in the 67 Nlike ions with 26≤Z≤92
Relativistic distortedwave collision strengths have been calculated for the 49 Δn=0 optically allowed transitions with n=2 in the 67 Nlike ions with nuclear charge number Z in the range 26≤Z≤92. The calculations were made for the four final, or scattered, electron energies E{sup ′}=0.20, 0.42, 0.80, and 1.40, where E{sup ′} is in units of Z{sub eff}{sup 2} Ry with Z{sub eff}=Z−5. In the present calculations, an improved “topup” method, which employs relativistic plane waves, was used to obtain the high partialwave contribution for each transition, in contrast to the partialrelativistic Coulomb–Bethe approximation used in the previous work by Zhangmore » 
Relativistic distortedwave collision strengths for the 16 Δn=0 optically allowed transitions with n=2 in the 67 Olike ions with 26≤Z≤92
Relativistic distortedwave collision strengths have been calculated for the 16 Δn=0 optically allowed transitions with n=2 in the 67 Olike ions with nuclear charge number Z in the range 26≤Z≤92. The calculations were made for the four final, or scattered, electron energies E{sup ′}=0.20,0.42,0.80, and 1.40, where E{sup ′} is in units of Z{sub eff}{sup 2} Ry with Z{sub eff}=Z−5.83. In the present calculations, an improved “topup” method, which employs relativistic plane waves, was used to obtain the high partialwave contribution for each transition, in contrast to the partialrelativistic Coulomb–Bethe approximation used in previous work by Zhang and Sampson [H.L.more »