Duncan Bossion
- Institut de Physique de Rennes (IPR)
- Department of Chemistry and Molecular Biology [Gothenburg]
Publications
Publications
Machine Learning for Astrochemistry: Multi-Layer Perceptron and ApplicationsSeminar at the Department of Space, Earth and Environment - Chalmers University of Technology, Nov 2025, Gothenburg (Sweden), Sweden |
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Cosmic Dust Growth in Astrophysical Environments: A Combined Dynamics and Machine Learning StudyPhysical and Chemical processes of astrophysical interest: astrochemistry in the JWST era (PCPAI), Jun 2025, Saint Florent - Corse, France |
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Non-adiabatic Dynamics using the Path-integral FormalismSeminar at the Institut des Sciences Chimiques de Rennes (ISCR) - Université de Rennes, May 2024, Rennes, France |
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Machine learning prediction of state-to-state rate constants for astrochemistryQuantum Reactive Scattering (QRS), Jun 2024, Istanbul (Turquie), Turkey |
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On the Impact of Atomic and Molecular Accretion on Cosmic Dust GrowthPhysique et Chimie du Milieu Interstellaire (PCMI), Oct 2024, Bordeaux, France |
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Dyncamique adiabatique pour l'astrochimie, développements méthodologiques pour la dynamique non-adiabatiqueSeminar at the Institue of Physics of Rennes - University of Rennes, Jan 2023, Rennes, France |
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Non-Adiabatic Mapping Dynamics in the phase space of SU(N) Lie groupACS Northeastern Regional Meeting, Oct 2022, Rochester, NY, United States |
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Activités de Recherche en Astrochimie et Développements MéthodologiquesSeminar at the Laboratoire de Chimie théorique (LCT) at Sorbonne University, May 2022, Paris, France |
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Non-adiabatic Dyncamics using the Path-integral FormalismSeminar at the Laboratoire de Physique et Chimie Théorique (LPCT) - Université de Lorraine, Feb 2022, Metz, France |
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The spin-mapping RPMD, a new approach to study non-adiabatic dynamicsAnnual GdR ThéMS meeting, Dec 2020, Metz, France |
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A ring polymer molecular dynamics study of low temperature insertion reactions for astrochemistryDynamics of Molecular Collisions XXVII, Jul 2019, Big Sky, MT, United States |
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Statistical behaviour of the HeH$^+$ + H $\rightarrow$ H$_2^+$ + He reaction, a quasi-classical and quantum statistical studyJournée SF2A, atelier PCMI, May 2019, Nice, France |
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Collisional excitation of H$_2$ by H atoms at high temperature for astrophysical applications22nd European Conference on the Dynamics of Molecular Systems, Aug 2018, Dinard, France |
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Quasi-classical and quantum study of atom-diatom collisions for high temperature regimePhysique et Chimie du Milieu Interstellaire, Jun 2018, Marseille, France |
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Collisional excitation of H$_2$ at high temperaturesPICS Collisional Excitation of Hydrides in the InterStellar Medium meeting, Aug 2018, Grenoble, France |
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State-to-state study of the D+H$_2$ reaction for the primordial UniverseGdR ThéMS meeting, Nov 2017, Metz, France |
SM-NRPMD: A Novel Method to Study Non-Adiabatic DynamicsACS Spring 2022 Bonding Through Chemistry, Mar 2022, San Diego, CA, United States |
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Non-adiabatic ring polymer molecular dynamics with spin mapping variables: A novel method to study non-adiabatic dynamicsACS Fall 2021 Resilience of Chemistry, Aug 2021, Atlanta, GA, United States |
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Ro-vibrational excitation of H$_2$ by H for high temperature regime22nd European Conference on the Dynamics of Molecular Systems, Aug 2018, Dinard, France |
Simulations numériques des collisions atome-molécule pour l'astrophysiqueRencontre utilisateurs du centre de calcul MESO@LR, Mar 2018, Montpellier, France |
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Ro-vibrational excitation of H$_2$ by H for high temperature regimePhysique et Chimie du Milieu Interstellaire, Jun 2018, Marseille, France |
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Simulations numériques de systèmes hamiltonien astrophysiques : collisions atome-molécule et orbites stellairesRencontre utilisateurs du centre de calcul MESO@LR, Dec 2018, Montpellier, France |
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General Formulas of the Structure Constants in the $\mathfrak{su}(N)$ Lie Algebra2024 |
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Théories et simulations de collisions moléculaires réactives pour la chimie primordialeAutre [cond-mat.other]. Université Montpellier, 2019. Français. ⟨NNT : 2019MONTS090⟩ |