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Desorption dynamics of interstellar molecule on amorphous solid water investigated by machine learning

Natsuki Watanabe1,2, Johannes Kästner3, Yuta Hori4

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This study introduces a new computational method, PaCS-MLP-MD, to simulate rare molecular events on interstellar ice surfaces. It reveals two distinct pathways for aminoacetonitrile (AAN) desorption from amorphous solid water (ASW).

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Area of Science:

  • Astrochemistry
  • Computational Chemistry
  • Surface Science

Background:

  • Interstellar amorphous solid water (ASW) surfaces are crucial for chemical evolution in molecular clouds.
  • Understanding molecular interactions with ASW is key to elucidating these chemical processes.
  • Accurate and efficient molecular dynamics (MD) simulations are needed to study ASW surface dynamics.

Purpose of the Study:

  • To develop and apply a novel computational scheme, PaCS-MLP-MD, for simulating rare-event dynamics on ASW.
  • To investigate the desorption mechanisms of aminoacetonitrile (AAN) from ASW surfaces.
  • To provide insights into molecular processes relevant to astrochemistry.

Main Methods:

  • Combined parallel cascade selection MD (PaCS-MD) with machine learning potential-based MD (MLP-MD) into a PaCS-MLP-MD framework.
  • Simulated desorption of AAN from an ASW surface model using PaCS-MLP-MD.
  • Performed unbiased MLP-MD simulations to study desorption and re-adsorption behaviors.

Main Results:

  • Identified two distinct AAN desorption pathways from ASW: amino-first and nitrile-first.
  • Revealed desorption and re-adsorption dynamics of AAN on the ASW surface through unbiased simulations.
  • Demonstrated the capability of PaCS-MLP-MD to explore complex surface reaction dynamics without external forces or temperature increases.

Conclusions:

  • The PaCS-MLP-MD method offers a robust framework for studying astrochemically relevant molecular processes on ASW.
  • The identified AAN desorption pathways contribute to a deeper understanding of surface chemistry in interstellar environments.
  • These findings enhance our knowledge of molecular interactions and evolution within molecular clouds.