Sodium 3s-3p far wing shapes induced by ground neon atoms

被引:0
|
作者
Sehab, F. [1 ]
Lamoudi, N. [1 ,2 ]
Alioua, K. [3 ]
Bouazza, M. T. [1 ,4 ,6 ]
Bouledroua, M. [5 ]
机构
[1] Badji Mokhtar Univ, Annaba, Algeria
[2] Lab Etud Surfaces & Interfaces Matiere Solide LESI, Annaba, Algeria
[3] Mohamed Cher Messaadia Univ, Lab Phys Matiere & Rayonnement, Souk Ahras, Algeria
[4] Badji Mokhtar Univ, Lab LAMA, Annaba, Algeria
[5] Badji Mokhtar Univ, Lab Phys Rayonnements, Annaba, Algeria
[6] Badji Mokhtar Univ, BP 12, Annaba, Algeria
关键词
Potential energy curve; pressure broadening; absorption coefficient; emission coefficient; satellite structure; BROWN DWARF; RESONANCE LINES; SPECTRA; PROFILES; POTASSIUM; RADIATION; LITHIUM; HELIUM; MODEL;
D O I
10.1080/00268976.2023.2249136
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
This study deals with the broadening of atomic sodium, evolving in a neon buffer gas, in the wavelength and temperature ranges 500--700nm500--700nm and 136--3000K136--3000K, respectively. The computed emission and absorption spectral profiles are based on the most recent potential energy curves and transition dipole moments. The required electronic Na(S-2) +Ne(S-1)+ and Na(P-2)+Ne(S-1) potentials are used from two different sets. Then the satellite structures in the blue wing are analysed quantum mechanically. The calculations show especially that the free-free transitions contribute most to the NaNe photoabsorption spectra and a satellite structure is observable beyond the temperature 402K402K around the wavelengths 550nm550nm depending on the used potential set. The obtained results showed good agreement with those already published.
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页数:8
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