Transition Energies, Oscillator Strengths, and Transition Probabilities of High-lying 1P O and 1D E States of Neon-like Ions

1996 ◽  
Vol 468 ◽  
pp. 445 ◽  
Author(s):  
A. K. Das
Keyword(s):  
Transition Probabilities ◽  
Oscillator Strengths ◽  
Transition Energies

Transition energies, transition probabilities and weighted oscillator strengths of He-like Al in hot and dense plasmas

2017 ◽  
Vol 92 (7) ◽  
pp. 075401 ◽  
Author(s):  
Xiang-Fu Li ◽  
Gang Jiang ◽  
Hong-Bin Wang ◽  
Miao Wu ◽  
Qian Sun
Keyword(s):  
Transition Probabilities ◽  
Oscillator Strengths ◽  
Transition Energies ◽  
Dense Plasmas

scholarly journals Extended theoretical transition data in C i–iv

2021 ◽  
Vol 502 (3) ◽  
pp. 3780-3799
Author(s):  
W Li ◽  
A M Amarsi ◽  
A Papoulia ◽  
J Ekman ◽  
P Jönsson
Keyword(s):  
Transition Probabilities ◽  
Energy Levels ◽  
Oscillator Strengths ◽  
Atomic Data ◽  
Internal Validation ◽  
Hartree Fock ◽  
Relativistic Configuration ◽  
The Difference ◽  
The One ◽  
Relative Differences

ABSTRACT Accurate atomic data are essential for opacity calculations and for abundance analyses of the Sun and other stars. The aim of this work is to provide accurate and extensive results of energy levels and transition data for C i–iv. The Multiconfiguration Dirac–Hartree–Fock and relativistic configuration interaction methods were used in this work. To improve the quality of the wavefunctions and reduce the relative differences between length and velocity forms for transition data involving high Rydberg states, alternative computational strategies were employed by imposing restrictions on the electron substitutions when constructing the orbital basis for each atom and ion. Transition data, for example, weighted oscillator strengths and transition probabilities, are given for radiative electric dipole (E1) transitions involving levels up to 1s22s22p6s for C i, up to 1s22s27f for C ii, up to 1s22s7f for C iii, and up to 1s28g for C iv. Using the difference between the transition rates in length and velocity gauges as an internal validation, the average uncertainties of all presented E1 transitions are estimated to be 8.05 per cent, 7.20 per cent, 1.77 per cent, and 0.28 per cent, respectively, for C i–iv. Extensive comparisons with available experimental and theoretical results are performed and good agreement is observed for most of the transitions. In addition, the C i data were employed in a re-analysis of the solar carbon abundance. The new transition data give a line-by-line dispersion similar to the one obtained when using transition data that are typically used in stellar spectroscopic applications today.

scholarly journals Laser-Induced Breakdown Spectroscopy for Determination of Spectral Fundamental Parameters

2020 ◽  
Vol 10 (14) ◽  
pp. 4973
Author(s):  
Sabrina Messaoud Aberkane ◽  
Ali Safi ◽  
Asia Botto ◽  
Beatrice Campanella ◽  
Stefano Legnaioli ◽  
...  
Keyword(s):  
Transition Probabilities ◽  
Oscillator Strengths ◽  
Stark Broadening ◽  
Future Perspectives ◽  
Fundamental Parameters ◽  
Breakdown Spectroscopy ◽  
Laser Induced Breakdown ◽  
And Shifts ◽  
Analytical Approaches

In this review, we report and critically discuss the application of LIBS for the determination of plasma-emission fundamental parameters, such as transition probabilities, oscillator strengths, Stark broadening and shifts, of the emission lines in the spectrum. The knowledge of these parameters is of paramount importance for plasma diagnostics or for quantitative analysis using calibration-free LIBS methods. In the first part, the theoretical basis of the analysis is laid down; in the second part, the main experimental and analytical approaches for the determination by LIBS of the spectral line spectroscopic parameters are presented. In the conclusion, the future perspectives of this kind of analysis are discussed.

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