Rotational de-excitation of N-protonated isocyanic acid (H2NCO+) by collision with He atoms

ABSTRACT Isocyanic acid protonated at nitrogen (H$_2$NCO$^+$) can help to understand the chemistry of [C,H,N,O] isomeric family as well as the determination of their abundance in the Sgr B2(N) and low-mass protostar L483 regions. New three-dimensional potential energy surface (3D-PES) for H$_2$NCO$^+$-He complex was constructed. The ab initio 3D-PES was computed by the use of explicitly correlated coupled cluster approach with single, double, and perturbative triple excitation (CCSD(T)-F12a) with augmented-correlation consistent-polarized valence triple zeta (aug-cc-pVTZ) Gaussian basis set. A global minimum with a well depth of 238.95 cm$^{-1}$ located at ($\Phi$ = 90$^\circ$, $\theta$ = 95$^\circ$, and R = 5.2 bohr) was observed. Rotational cross-sections were calculated for total energy up to 1000 cm$^{-1}$ using coupled states approach. Thermal rate coefficients were estimated until temperature of 200 K. Propensity rules favouring $|\Delta J| = |\Delta K_c| = 1$ with $|\Delta K_a|$ = 0 transitions were found for both para and ortho-H$_2$NCO$^+$.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-10-14
DOI
https://doi.org/10.1093/mnras/staf1761
Primary Topic
Molecular Spectroscopy and Structure
Type
article
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article

Rotational de-excitation of N-protonated isocyanic acid (H2NCO+) by collision with He atoms

Manel Naouai, Abdelhak Jrad
Monthly Notices of the Royal Astronomical Society
Molecular Spectroscopy and Structure
article

Rotational de-excitation of N-protonated isocyanic acid (H2NCO+) by collision with He atoms

Manel Naouai, Abdelhak Jrad
article en

Abstract

ABSTRACT Isocyanic acid protonated at nitrogen (H$_2$NCO$^+$) can help to understand the chemistry of [C,H,N,O] isomeric family as well as the determination of their abundance in the Sgr B2(N) and low-mass protostar L483 regions. New three-dimensional potential energy surface (3D-PES) for H$_2$NCO$^+$-He complex was constructed. The ab initio 3D-PES was computed by the use of explicitly correlated coupled cluster approach with single, double, and perturbative triple excitation (CCSD(T)-F12a) with augmented-correlation consistent-polarized valence triple zeta (aug-cc-pVTZ) Gaussian basis set. A global minimum with a well depth of 238.95 cm$^{-1}$ located at ($\Phi$ = 90$^\circ$, $\theta$ = 95$^\circ$, and R = 5.2 bohr) was observed. Rotational cross-sections were calculated for total energy up to 1000 cm$^{-1}$ using coupled states approach. Thermal rate coefficients were estimated until temperature of 200 K. Propensity rules favouring $|\Delta J| = |\Delta K_c| = 1$ with $|\Delta K_a|$ = 0 transitions were found for both para and ortho-H$_2$NCO$^+$.

Monthly Notices of the Royal Astronomical SocietyVol. 544(1)
Tunis University (TN), Institut Supérieur des Études Technologiques de Nabeul (TN), Institut Préparatoire aux Études d'Ingénieurs de Monastir (TN), University of Jendouba (TN), Tunis El Manar University (TN)
Openalex Percentile: Top 73%
Molecular Spectroscopy and Structure
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Rotational de-excitation of N-protonated isocyanic acid (H2NCO+) by collision with He atoms — Manel Naouai, Abdelhak Jrad · Monthly Notices of the Royal Astronomical Society (2025) | TGRS Research Map | TGRS