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Extreme ultraviolet and x-ray transition wavelengths in Rb XXIV |
Indu Khatria, Arun Goyala, Sunny Aggarwala c, A. K. Singhb, Man Mohana |
a Department of Physics and Astrophysics, University of Delhi, Delhi-110007, India; b Department of Physics, D.D.U. College, University of Delhi, Delhi-110015, India; c Department of Physics, Shyamlal College, University of Delhi, Delhi-110032, India |
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Abstract Energy levels, radiative rates, oscillator strengths and line strengths are reported for transitions among the lowest 97 levels of the (1s22s22p6) 3s23p2, 3s23p3d, 3s3p3, 3p4, 3s3p23d, and 3s23d2 configurations of Rb XXIV. A multiconfiguration Dirac-Fock (MCDF) method is adopted for the calculations. Radiative rates, oscillator strengths, and line strengths are provided for all electric dipole (E1), magnetic dipole (M1), electric quadrupole (E2), and magnetic quadrupole (M2) transitions from the ground level to all 97 levels, although calculations are performed for a much larger number of levels. To achieve the accuracy of the data, comparisons are provided with similar data obtained from the Flexible Atomic Code (FAC) and also with the available theoretical and experimental results. Our energy levels are found to be accurate to better than 1.2%. Wavelengths calculated are found to lie in EUV (extreme ultraviolet) and x-ray regions. Additionally, lifetimes for all 97 levels are obtained for the first time.
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Received: 16 February 2015
Revised: 20 May 2015
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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Fund: The authors, Indu Khatri and Arun Goyal, were supported by the U. G. C., India for their Junior Research Fellowship and Man Mohan by the U.G.C. for Basic Science Research Fellowship. |
Corresponding Authors:
Arun Goyal
E-mail: arun.goyal.du@gmail.com
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Cite this article:
Indu Khatri, Arun Goyal, Sunny Aggarwal, A. K. Singh, Man Mohan Extreme ultraviolet and x-ray transition wavelengths in Rb XXIV 2015 Chin. Phys. B 24 103202
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