Article (Scientific journals)
Robust Binding Energy Distribution Sampling on Amorphous Solid Water Models. Method testing and validation with NH3, CO and CH4
Groyne, Maria; Champagne, Benoît; Baijot, Cédric et al.
2025In Astronomy and Astrophysics, 698 (A284)
Peer Reviewed verified by ORBi
 

Files


Full Text
aa55097-25.pdf
Publisher postprint (5.1 MB) Creative Commons License - Attribution
22 pages, 27 Figures
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
astro-ph.IM
Abstract :
[en] The astrochemically efficient icy mantles surrounding dust grains in molecular clouds have been shown to be of a water-rich amorphous nature. This therefore implies a distribution of binding energies (BE) per species instead of a single value. Methods proposed so far for inferring BE and their distributions on amorphous ices rely on different approaches and approximations, leading to disparate results or BE dispersions with partially overlapping ranges. This work aims to develop a method based on a structurally reliable ice model and a statistically and physico-chemically robust approach for BE distribution inference, with the aim to be applicable to various relevant interstellar species. A multiscale computational approach is presented, with a Molecular Dynamics (MD) Heat & Quench protocol for the amorphous water ice model, and an ONIOM(B3LYP-D3(BJ)/6-311+G**:GFN2-xtb) scheme for the BE inference, with a prime emphasis onto the BE/real system size convergence. The sampling of the binding configurations is twofold, exploring both regularly spaced binding sites, as well as various adsorbate-to-substrate orientations on each locally distinct site. This second source of BE diversity accounts for the local roughness of the potential energy landscape of the substrate. Three different adsorbate test cases are considered, i.e. NH3, CO and CH4, owing to their significance in dust icy mantles, and their distinct binding behavior with water ices. The BE distributions for NH3, CO and CH4 have been inferred, with converged statistics. The distribution for NH3 is better represented by a double Gaussian component profile. Three starting adsorbate orientations per site are required to reach convergence for both Gaussian components of NH3, while 2 orientations are sufficient for CO, and one unique for CH4 (symmetric). Further geometrical and molecular surrounding insights have been provided. These results encompass previously reported results.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Groyne, Maria  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Multi-wavelength Extragalactic and Galactic Astrophysics (MEGA)
Champagne, Benoît
Baijot, Cédric  ;  Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
De Becker, Michaël  ;  Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Sciences spatiales
Language :
English
Title :
Robust Binding Energy Distribution Sampling on Amorphous Solid Water Models. Method testing and validation with NH3, CO and CH4
Publication date :
24 June 2025
Journal title :
Astronomy and Astrophysics
ISSN :
0004-6361
eISSN :
1432-0746
Publisher :
EDP Sciences, Les Ulis, France
Volume :
698
Issue :
A284
Peer reviewed :
Peer Reviewed verified by ORBi
Tags :
CÉCI : Consortium des Équipements de Calcul Intensif
Funders :
F.R.S.-FNRS - Fund for Scientific Research
Commentary :
Published in A&A 22 pages, 27 Figures on June 24, 2025 ( https://doi.org/10.1051/0004-6361/202555097)
Available on ORBi :
since 28 April 2025

Statistics


Number of views
97 (6 by ULiège)
Number of downloads
37 (0 by ULiège)

Scopus citations®
 
3
Scopus citations®
without self-citations
3
OpenCitations
 
0
OpenAlex citations
 
4

Bibliography


Similar publications



Contact ORBi