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New atomic data for Kr XXXV useful in fusion plasma |
Sunny Aggarwal, Jagjit Singh, Man Mohan |
Department of Physics and Astrophysics, University of Delhi, Delhi 110007, India |
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Abstract Energy levels and emission line wavelengths of high-Z materials are useful for impurity diagnostics due to its potential application in the next generation fusion devices. For this purpose, we have calculated the fine structural energies of the 67 levels belonging to the 1s2, 1s2l, 1s3l, 1s4l, 1s5l, and 1s6l configurations of Kr XXXV using GRASP (general purpose relativistic atomic structure package) code. Additionally, we have reported the transition probabilities, oscillator strengths, line strengths, and transition wavelengths for some electric dipole (E1) transitions among these levels. We predict new energy levels and radiative rates, which have not been reported experimentally or theoretically, forming the basis for future experimental work.
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Received: 16 September 2012
Revised: 27 September 2012
Accepted manuscript online:
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PACS:
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32.70.Cs
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(Oscillator strengths, lifetimes, transition moments)
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Corresponding Authors:
Sunny Aggarwal
E-mail: sunny.kmc87@gmail.com
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Cite this article:
Sunny Aggarwal, Jagjit Singh, Man Mohan New atomic data for Kr XXXV useful in fusion plasma 2013 Chin. Phys. B 22 033201
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[1] |
Lee P, Leiber A J, Pradhan A K and Xu Y 1986 Phys. Rev. A 34 3210
|
[2] |
Mohan M, Aggarwal S, Singh J and Jha A K S (Communicated)
|
[3] |
Zhang L, Jiang G, Hao L and Deng B 2011 Phys. Scr. 83 025302
|
[4] |
Griffin D C and Balance C P 2009 J. Phys. B 42 235201
|
[5] |
Natarajan A and Natarajan L 2008 JQSRT 109 2281
|
[6] |
Natarajan L and Natarajan A 2009 Phys. Rev. A 79 062513
|
[7] |
Cheng K T 1996 private communication
|
[8] |
Cheng K T and Chen M H 2000 Phys. Rev. A 61 044503
|
[9] |
Drake G W F 1985 (Unpublished)
|
[10] |
Vainshtein L A and Safronova U I 1985 (Unpublished)
|
[11] |
Widmann K, Beiersdorfer P, Decaux V and Bitter M 1996 Phys. Rev. A 53 2200
|
[12] |
Martin S, Denis A, Buchet-Poulizac M C, Buchet J P and Désesquelles J 1990 Phys. Rev. A 42 6570
|
[13] |
Indelicato P, Briand J P and Tavernier M 1986 Z. Phys. D 2 249
|
[14] |
Briand J P, Indelicato P, Tavernier M, Gorceix O, Liesen D, Beyer H F, Liu B, Warczak A and Desclaux J P 1984 Z. Phys. A 318 1
|
[15] |
Gould H and Marrus R 1976 Plenum 1 305
|
[16] |
Büttner R, Kraus B, Nicolai M, Schartner K H, Folkmann F, Mokler P H and Möller G 1993 AIP Conf. Proc. 274 423
|
[17] |
Grant I P, Mckenzie B J, Norrington P H, Mayers D F and Pyper N C 1980 Comput. Phys. Commun. 21 207
|
[18] |
Saloman E B 2007 J. Phys. Chem. Ref. Data 36 215
|
[19] |
Hibbert A 2004 Phys. Scr. T112 207
|
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