Theoretical description of interstellar ...
Type de document :
Communication dans un congrès avec actes
Titre :
Theoretical description of interstellar ices from a multimethod approach
Auteur(s) :
Michoulier, Eric [Auteur]
Physico-Chimie Moléculaire Théorique [PCMT]
Mascetti, Joelle [Auteur]
Institut des Sciences Moléculaires [ISM]
Noble, Jennifer [Auteur]
Physique des interactions ioniques et moléculaires [PIIM]
Toubin, Céline [Orateur]
Physico-Chimie Moléculaire Théorique [PCMT]
Simon, Aude [Auteur]
Modélisation, Agrégats, Dynamique (LCPQ) [MAD]
Laboratoire de Chimie et Physique Quantiques [LCPQ]
Physico-Chimie Moléculaire Théorique [PCMT]
Mascetti, Joelle [Auteur]
Institut des Sciences Moléculaires [ISM]
Noble, Jennifer [Auteur]
Physique des interactions ioniques et moléculaires [PIIM]
Toubin, Céline [Orateur]
Physico-Chimie Moléculaire Théorique [PCMT]
Simon, Aude [Auteur]
Modélisation, Agrégats, Dynamique (LCPQ) [MAD]
Laboratoire de Chimie et Physique Quantiques [LCPQ]
Titre de la manifestation scientifique :
Atelier-glaces : Les glaces astrophysiques: observations, modèles, expériences de laboratoires
Ville :
Paris
Pays :
France
Date de début de la manifestation scientifique :
2019-10-03
Date de publication :
2019-10-03
Discipline(s) HAL :
Chimie/Chimie théorique et/ou physique
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Physique [physics]/Physique [physics]/Chimie-Physique [physics.chem-ph]
Résumé en anglais : [en]
Even if the ISM remains a cold environment with only few energy available, dynamics effects cannot be neglected since the surface state may be significantly altered due to thermal energy dissipation. It is possible to carry ...
Lire la suite >Even if the ISM remains a cold environment with only few energy available, dynamics effects cannot be neglected since the surface state may be significantly altered due to thermal energy dissipation. It is possible to carry electronic structure calculations on reduced and distorted structures that may reproduce somehow a thermally relaxed surface. Classical molecular dynamics based on a semi-empirical potential remains a method of choice to account for explicit dynamical effects and for large scale surfaces. Within the classical description of the intermolecular forces, only physisorption is accessible. This limitation can be overcome through the combination of dynamics/force field simulations and Self-consistent charge density functional tight binding (SCC-DFTB) calculations. This will be illustrated in the case of the adsorption of PAHs on crystalline and amorphous ices. We will present a complete description of PAH-ice interaction in the ground electronic state at low temperature, providing the binding energies and barrier heights necessary to the on-going improvement of astrochemical models.Lire moins >
Lire la suite >Even if the ISM remains a cold environment with only few energy available, dynamics effects cannot be neglected since the surface state may be significantly altered due to thermal energy dissipation. It is possible to carry electronic structure calculations on reduced and distorted structures that may reproduce somehow a thermally relaxed surface. Classical molecular dynamics based on a semi-empirical potential remains a method of choice to account for explicit dynamical effects and for large scale surfaces. Within the classical description of the intermolecular forces, only physisorption is accessible. This limitation can be overcome through the combination of dynamics/force field simulations and Self-consistent charge density functional tight binding (SCC-DFTB) calculations. This will be illustrated in the case of the adsorption of PAHs on crystalline and amorphous ices. We will present a complete description of PAH-ice interaction in the ground electronic state at low temperature, providing the binding energies and barrier heights necessary to the on-going improvement of astrochemical models.Lire moins >
Langue :
Anglais
Comité de lecture :
Oui
Audience :
Nationale
Vulgarisation :
Non
Source :