Rate coefficients for the process CS(v) + He -> CS(v-Delta v) + He with Delta v = 1, 2, 3 and for v up to 45 were calculated in the 80-5000 K temperature using a mixed quantum-classical (MQC) method. The dataset was then completed using a Neural Network (NN) model, trained on the MQC rate coefficients. The reliability of the MQC method was first verified by comparing the new MQC results with initially state-selected ro-vibrational rate coefficients up to v = 2 computed with the vibrational close-coupling infinite-order sudden (VCC-IOS) method [F. Lique and A. Spielfiedel, Astron. Astrophys., 2007, 462, 1179] employing the same potential energy surface (PES). To enable calculations for higher vibrationally excited states, a new analytical PES was developed that is suitable even under large bond distortions.

Vibrational relaxation rate coefficients in CS-He collisions up to the dissociation limit: mixed quantum-classical calculations and neural network predictions

Pezzella, M;Storchi, L;Coletti, C
2026-01-01

Abstract

Rate coefficients for the process CS(v) + He -> CS(v-Delta v) + He with Delta v = 1, 2, 3 and for v up to 45 were calculated in the 80-5000 K temperature using a mixed quantum-classical (MQC) method. The dataset was then completed using a Neural Network (NN) model, trained on the MQC rate coefficients. The reliability of the MQC method was first verified by comparing the new MQC results with initially state-selected ro-vibrational rate coefficients up to v = 2 computed with the vibrational close-coupling infinite-order sudden (VCC-IOS) method [F. Lique and A. Spielfiedel, Astron. Astrophys., 2007, 462, 1179] employing the same potential energy surface (PES). To enable calculations for higher vibrationally excited states, a new analytical PES was developed that is suitable even under large bond distortions.
2026
Inglese
28
4
2920
2931
12
7
info:eu-repo/semantics/article
262
Pezzella, M; Pirani, F; Bartolomei, M; Hong, Qz; Lique, F; Storchi, L; Coletti, C
1 Contributo su Rivista::1.1 Articolo in rivista
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   Parallelizzazione e Porting su GPU di Codici Scientifici
   PaGUSci
   Istituto Nazionale di Astrofisica
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11564/872153
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