H-bond symmetrization in high pressure methane hydrate

International audience First-principle molecular dynamics simulations of methane hydrate MH-III, including the quantum properties of the hydrogen nuclei, were carried out at pressures in the 5-65 GPa range, in order to observe the H-bond symmetrization at high pressure and at room temperature. Accor...

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Bibliographic Details
Published in:Journal of Physics: Conference Series
Main Authors: Schaack, Sofiane, Depondt, Philippe, Finocchi, Fabio
Other Authors: Oxydes en basses dimensions (INSP-E9), Institut des Nanosciences de Paris (INSP), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)
Format: Conference Object
Language:English
Published: HAL CCSD 2016
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Online Access:https://hal.archives-ouvertes.fr/hal-01985288
https://hal.archives-ouvertes.fr/hal-01985288/document
https://hal.archives-ouvertes.fr/hal-01985288/file/Schaack_2018_J._Phys.__Conf._Ser._1136_012018.pdf
https://doi.org/10.1088/1742-6596/1136/1/012018
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Summary:International audience First-principle molecular dynamics simulations of methane hydrate MH-III, including the quantum properties of the hydrogen nuclei, were carried out at pressures in the 5-65 GPa range, in order to observe the H-bond symmetrization at high pressure and at room temperature. According to our simulations, the symmetrization transition takes place around 40 GPa and is little dependent on isotope substitution. We find that, consistently with the rather complex crystal structure of MH-III, the transition is much more convoluted in the hydrate than in ices VII and X. In methane hydrate, due to the presence of non equivalent O ions with distinct O-O distances, the dissimilar H bonds symmetrize in a pressure domain rather than at a single critical pressure.