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Chin. Phys. B, 2015, Vol. 24(12): 123201    DOI: 10.1088/1674-1056/24/12/123201
ATOMIC AND MOLECULAR PHYSICS Prev   Next  

Comment on “Relativistic atomic data for W XLVII” by S. Aggarwal et al. [Chin. Phys. B 24 (2015) 053201]

Kanti M. Aggarwal
Astrophysics Research Center, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, Northern Ireland, UK
Abstract  Recently, S. Aggarwal et al. [Chin. Phys. B 24 (2015) 053201] reported energy levels, radiative rates, and lifetimes for the lowest 148 levels belonging to the 3s23p, 3s3p2, 3s23d, 3s3p3d, 3p3, 3p23d, 3s3d2, 3p3d2, and 3d3 configurations of Al-like tungsten. While their calculated energies for the levels and the radiative rates for transitions are correct, the reported results for lifetimes are completely wrong. According to our calculations, errors in their reported lifetimes are up to 14 orders of magnitude for over 90% of the levels. Here we report the correct lifetimes and explain the reasons for discrepancies.
Keywords:  energy levels      radiative rates      lifetimes      Al-like tungsten  
Received:  20 August 2015      Revised:  09 October 2015      Accepted manuscript online: 
PACS:  32.70.Cs (Oscillator strengths, lifetimes, transition moments)  
  95.30.Ky (Atomic and molecular data, spectra, and spectralparameters (opacities, rotation constants, line identification, oscillator strengths, gf values, transition probabilities, etc.))  
Corresponding Authors:  Kanti M. Aggarwal     E-mail:  K.Aggarwal@qub.ac.uk

Cite this article: 

Kanti M. Aggarwal Comment on “Relativistic atomic data for W XLVII” by S. Aggarwal et al. [Chin. Phys. B 24 (2015) 053201] 2015 Chin. Phys. B 24 123201

[1] Aggarwal K M and Keenan F P 2013 Fusion Sci. Tech. 63 363
[2] Aggarwal S, Jha A K S, Khatri I, Singh N and Mohan M 2015 Chin. Phys. B 24 053201
[3] Aggarwal K M and Keenan F P 2015 At. Data Nucl. Data Tables, submitted for publication
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