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NGFSRDW databaseclick to expand or collapse

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Data Group [Ar]: The cross sections for excitation of the fine-structure levels of Ar in the database have been calculated by the
Relativistic Distorted Wave (RDW) method. See R K Gangwar, L Sharma, R Srivastava and A D Stauffer,
J. Appl. Phys. 111, 053307 (2012) for a general description plus an application of these cross sections to modeling
of Ar plasmas. This paper also contains calculations of cross sections for the following transitions:
Ar 3p^5 4s (radiative levels) - 3p^5 4p
Ar 3p^5 4s (transitions among fine-structure levels)
Ar 3p^5 4p (transitions among fine-structure levels)
References for other transtions.
Some of these paper include analytic fits to the higher energy cross sections.
Ar 3p^6 - 3p^5 4s, M A Khakoo, P Vandeventer, J G Childers, I Kanik, C J Fontes, K Bartschat, V Zeman, D H Madison,
S Saxena, R Srivastava and A D Stauffer, J. Phys. B 37, 247 (2004)
Ar 3p^6 - 3p^5 4p, Savinder Kaur, R Srivastava, R P McEachran and A D Stauffer, J. Phys. B 31, 4833 (1998)
Ar 3p^6 - 3p^5 3d, 5s, 5p, R K Gangwar, L Sharma, R Srivastava and A D Stauffer, Phys. Rev. A 81, 052707 (2010)
Ar 3p^5 4s (metastable levels) - 3p^5 4p, R Srivastava, A D Stauffer and L Sharma, Phys. Rev. A 74, 012715 (2006)
Ar 3p^5 4s (metastable levels) - 3p^5 5p, L Sharma, R Srivastava and A D Stauffer, Phys. Rev. A 76, 024701 (2007).

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e / Ar(3p5 4s J = 0 1s3)