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Published on: April 12, 2019
Hydrogen Recombination and Dimer Formation on Graphite from Ab Initio Molecular Dynamics Simulations
S Casolo1, G F Tantardini1,2, R Martinazzo1,2
1Dipartimento di Chimica, Università degli Studi di Milano , via Golgi 19, 20133 Milan, Italy.
Eley-Rideal molecular hydrogen formation on graphite is hindered at low energies relevant to interstellar chemistry due to projectile steering. Efficient dimer formation occurs only at higher energies, not found in the interstellar medium.
Area of Science:
- Astrochemistry
- Surface Science
- Chemical Physics
Background:
- Molecular hydrogen (H2) formation is crucial for the interstellar medium (ISM).
- The Eley-Rideal mechanism is a proposed pathway for H2 formation on dust grains.
- Understanding H2 formation on graphite is key to astrochemistry and plasma physics.
Purpose of the Study:
- Investigate Eley-Rideal H2 formation on graphite surfaces.
- Determine the energy range for H2 formation relevant to ISM and cold plasma experiments.
- Analyze projectile steering effects and dimer formation pathways.
Main Methods:
- Ab initio molecular dynamics simulations.
- Calculations of reaction cross sections.
- Analysis of ro-vibrational product populations.
Main Results:
- Projectile steering effects significantly inhibit dimer formation at low energies (0.02-1 eV).
- Efficient ortho and para dimer formation observed only at energies too high for ISM relevance.
- Simulated adsorbate configurations match experimental scanning tunneling microscopy observations.
Conclusions:
- The Eley-Rideal mechanism is unlikely to be a dominant pathway for H2 synthesis in the ISM under studied conditions.
- Computed data align well with experimental findings for H2 formation and surface interactions.
- This study refines our understanding of H2 formation on interstellar dust analogs.
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