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Energy levels and radiative rates for transitions in Ti X

2013/07/10 by K. M. Aggarwal, KM Aggarwal, Aggarwal, KM +3 · 1 citation
Engineering · Physics and Astronomy · #Atomic Physics (physics.atom-ph) #Atomic and Molecular Physics #FOS: Physical sciences #Laser-induced spectroscopy and plasma #X-ray Spectroscopy and Fluorescence Analysis #physics.atom-ph

paper · pdf · doi:10.48550/arxiv.1307.2732

13p Text and 8 Tables will appear in Physica Scripta 88 (2013) xxxxxx. arXiv admin note: substantial text overlap with arXiv:1307.2471

arxiv created 2013/07/10 · openalex publication_date 2013/07/10 · arxiv updated 2013/07/11 · openalex created_date 2022/10/03 · openalex updated_date 2026/07/28

Abstract

We report calculations of energy levels, radiative rates, oscillator strengths and line strengths for transitions among the lowest 345 levels of Ti X. These include 146 levels of the n ≤ 3 configurations and 86 of 3s2 4ℓ, 3s2 5ℓ and 3s3p4ℓ, plus some of the 3s2 6ℓ, 3p2 4ℓ and 3s3p5ℓ levels. The general-purpose relativistic atomic structure package (\sc grasp) and flexible atomic code (\sc fac) are 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 among the 345 levels, although calculations have been performed for a much larger number of levels. Comparisons are made with existing results and the accuracy of the data is assessed. Additionally, lifetimes for all 345 levels are listed. Extensive comparisons of lifetimes are made for the lowest 40 levels, for which discrepancies with recent theoretical work are up to 30%. Discrepancies in lifetimes are even larger, up to a factor of four, for higher excited levels. Furthermore, the effect of large CI is found to be insignificant for both the energies and lifetimes for the lowest 40 levels of Ti X which belong to the 3s23p, 3s3p2, 3s23d, 3p3 and 3s3p3d configurations. However, the contribution of CI is more appreciable for the energy levels and radiative rates among higher excited levels. Our listed energy levels are estimated to be accurate to better than 1% (within 0.1 Ryd), whereas results for other parameters are probably accurate to better than 20%.

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