Temperature-Dependent Line-Broadening Effects in CO2 Caused by Ar

被引:2
|
作者
Salem, Jamel [1 ]
Tobias, Roland [2 ]
Csaszar, Attila G. [2 ,3 ]
Al-Mogren, Muneerah Mogren [4 ]
Jaidane, Nejm-Edine [5 ]
Hochlaf, Majdi [6 ]
机构
[1] Univ Gafsa, Fac Sci, Lab Technol, Energie Mat Innovants, Sidi Ahmed Zarroug 2112, Gafsa, Tunisia
[2] Eotvos Lorand Univ, Inst Chem, Lab Mol Struct & Dynam, Pazmany Peter Setany 1-A, H-1117 Budapest, Hungary
[3] HUN REN ELTE Complex Chem Syst Res Grp, POB 32, Budapest 112, Hungary
[4] King Saud Univ, Coll Sci, Dept Chem, POB 2455, Riyadh 11451, Saudi Arabia
[5] Univ Tunis Al Manar, Lab Spect Atom Mol & Applicat LSAMA, Tunis, Tunisia
[6] Univ Gustave Eiffel, COSYS IMSE, 5 Bd Descartes, F-77454 Champs Sur Marne, France
关键词
temperature-dependent line broadening parameters; Ar-broadened CO2 rovibrational transitions; interaction potential energy surface; modified Robert-Bonamy approach; generalized power-law model; HALF-WIDTHS; ENERGY-TRANSFER; RAMAN LINES; TRANSITIONS; INTENSITIES; SHIFTS; N-2; LINEWIDTHS; MOLECULES; DIPOLE;
D O I
10.1002/cphc.202300467
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 computational study of line-broadening effects is based on an accurate, analytical representation of the intermonomer potential energy surface (PES) of the CO2 & sdot; Ar van der Waals (vdW) complex. The PES is employed to compute collisional broadening coefficients for rovibrational lines of CO2 perturbed by Ar. The semiclassical computations are performed using the modified Robert-Bonamy approach, including real and imaginary terms, and the exact trajectory model. The lines investigated are in the 10001 <- 00011, 01101 <- 00001, 00011 <- 00001, and 00031 <- 00001 vibrational bands and the computations are repeated at multiple temperatures. The computed results are in good agreement with the available experimental values, validating both the intermonomer PES developed and the methodology used. For lines in the 01101 <- 00001 band of CO2, temperature-dependent Ar-broadening coefficients are reported for the first time. The parameters presented should prove useful, among other applications, for the accurate experimental determination of CO2 and Ar abundances in planetary atmospheres.
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页数:10
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