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Rotational excitation of 36ArH+ by He at low temperature.

Authors :
Bop, Cheikh T.
Hammami, K.
Niane, A.
Faye, N. A. B.
Jaïdane, N.
Source :
Monthly Notices of the Royal Astronomical Society; 2/11/2017, Vol. 465 Issue 1, p1137-1143, 7p
Publication Year :
2017

Abstract

In this paper, we focus on the determination of the rotational excitation rate coefficients of the first observed molecule containing noble gas <superscript>36</superscript>ArH<superscript>+</superscript> isotope by He. Hence, we present the first potential energy surface (PES) of ArH<superscript>+</superscript> --He van der Waals system. The interaction PES of the ArH<superscript>+</superscript> (X¹ Σ<superscript>)+</superscript>-He(¹S) complex is calculated by the ab initio explicitly correlated coupled cluster with single, double, and perturbative triple excitation (CCSD(T)-F12) method in connection with the augmented correlation consistent triple zeta Gaussian basis (aug-cc-pVTZ). The interaction potential presents two global minima of 708.00 and 172.98 cm<superscript>-1</superscript> below the ArH<superscript>+</superscript> (X¹ Σ <superscript>+</superscript>)-He(¹S) dissociation limit. Using the PES obtained, we have computed integral inelastic cross-sections in the close-coupling approach among the first 11 rotational levels of ArH<superscript>+</superscript> for energies up to 2500 cm<superscript>-1</superscript>. Downward rate coefficients were determined at low temperature (T ≤ 300 K). It is expected that the data worked out in this study may be beneficial for further astrophysical investigations as well as laboratory experiments. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
465
Issue :
1
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
120577760
Full Text :
https://doi.org/10.1093/mnras/stw2809