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Rate constants for a reactive system of astrophysical interest: a statistical study of CH(2)().

PubMed
Authors: González-Lezana T, Konings M, Loreau J, Lique F, Sil M, Faure A

Year

2026

Paper ID

10206

Status

Peer-reviewed

Abstract Read

~2 min

Abstract Words

115

Citations

N/A

Abstract

A systematic investigation on the different processes involving formation, destruction and (de)excitation of specific rovibrational states of CH has been carried out based on statistical approaches. Thus, reactive collisions between C(P) and H(, ) and between CH(, ) and H for a large number of state-to-state transitions have been studied using a statistical quantum method and a statistical adiabatic channel model. The capabilities of such techniques for the study of the title system are discussed with comparisons to previous quantum mechanical results and experimental data. Integral cross sections as a function of the energy and rate constants in terms of the temperature (up to 1500 K) are obtained and numerical data for astrophysical purposes are provided.

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Current Paper #10206 #69596 Comprehensive pKa Data Augmenta... #69589 An integrated ultrahigh vacuum ... #69558 Analyzing Initialization Strate... #69553 VQE as Initial State Preparatio...

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