Bulletin of the American Physical Society
2024 APS March Meeting
Monday–Friday, March 4–8, 2024; Minneapolis & Virtual
Session NN00: Virtual Poster Session III (6:30am-8:00am CST)
6:30 AM,
Thursday, March 7, 2024
Chair: Abdullah AlShuaibi, Cornell University; Apurba Paul, University of Notre Dame; Jonte Hance, Newcastle University
Abstract: NN00.00045 : High pressure-temperature superionic states of P-3 brucite [Mg(OH)2] promoting enhanced protonic conductivity*
Presenter:
Sudip Kumar Mondal
(Department of Physics, Jadavpur University)
Authors:
Sudip Kumar Mondal
(Department of Physics, Jadavpur University)
Pratik Kumar Das
(IIESTS)
Nibir Mandal
(Department of Geological Sciences, Jadavpur University)
Brucite is an archetype dense hydroxide mineral, belonging to ternary MgO-SiO2-H2O system, which can host a significant amount of water in the form of OH-. The consideration of brucite in H-circulation is thus of crucial importance as the dense hydrous silicates1 cannot account for the observed mantle conductivity. Using ab initio molecular dynamics simulations, we investigate the diffusion of H+(proton) in high-pressure P-3 polymorph of brucite in a combined high pressure (p)–temperature (T) range of 10-85 GPa and 1250-2000K. We observe vigorous proton diffusion at elevated p-T resulting in a liquid state of the H-sublattice, within solid Mg-O sublattice, generating the superionic states in brucite. This study also reveals an unusual pressure-dependent proton migration characterized by maximum H+-diffusion in the pressure range of 72-76 GPa along the isotherms. The mobility of H+ is found to be strongly anisotropic, allowing no transport across the MgO6-octahedral layers i.e. along c-axis. The liquid state of the protonic sublattice yields a quasi-2D layer of fast H+ causing a drastic enhancement in the electrical conductivity of P-3 brucite. Comparison of our calculated conductivity with ex-situ geophysical data2,3 indicates the possible brucite abundance to explain high-conductive zones in the deep mantle of earth.
1Hirschmann & Kohlstedt Phys. Today 65 40–5 2012
2Constable & Constable, Geochem. Geophys. Geosystems 5 1–15 2004
3Civet et al., Geophys. Res. Lett. 42 3338–46 2015
*SKM acknowldegs DST.
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