TY - JOUR
T1 - Post-stishovite transition in hydrous aluminous SiO2
AU - Umemoto, Koichiro
AU - Kawamura, Katsuyuki
AU - Hirose, Kei
AU - Wentzcovitch, Renata M.
N1 - Funding Information:
The authors thank David Kohlstedt, Justin Revenaugh, and George Helffrich for useful discussions. This work was supported by NSF under Grants EAR-1161023 and EAR-1348066 . Computations were performed at the Minnesota Supercomputing Institute (MSI) and in the Blue Waters system at NCSA.
Publisher Copyright:
© 2016 Elsevier B.V.
PY - 2016/6/1
Y1 - 2016/6/1
N2 - Lakshtanov et al. (2007) showed that incorporation of aluminum and some water into SiO2 significantly reduces the post-stishovite transition pressure in SiO2. This discovery suggested that the ferroelastic post-stishovite transition in subducted MORB crust could be the source of reflectors/scatterers with low shear velocities observed in the mid to upper lower mantle. A few years later, a similar effect was observed in anhydrous Al-bearing silica. In this paper, we show by first principles static calculations and by molecular dynamics using inter-atomic potentials that hydrogen bonds and hydrogen mobility play a crucial role in lowering the post-stishovite transition pressure. A cooperative redistribution of hydrogen atoms is the main mechanism responsible for the transition pressure reduction in hydrous aluminous stishovite. The effect is enhanced by increasing hydrogen concentration. This perspective suggests a potential relationship between the depth of seismic scatterers and the water content in stishovite.
AB - Lakshtanov et al. (2007) showed that incorporation of aluminum and some water into SiO2 significantly reduces the post-stishovite transition pressure in SiO2. This discovery suggested that the ferroelastic post-stishovite transition in subducted MORB crust could be the source of reflectors/scatterers with low shear velocities observed in the mid to upper lower mantle. A few years later, a similar effect was observed in anhydrous Al-bearing silica. In this paper, we show by first principles static calculations and by molecular dynamics using inter-atomic potentials that hydrogen bonds and hydrogen mobility play a crucial role in lowering the post-stishovite transition pressure. A cooperative redistribution of hydrogen atoms is the main mechanism responsible for the transition pressure reduction in hydrous aluminous stishovite. The effect is enhanced by increasing hydrogen concentration. This perspective suggests a potential relationship between the depth of seismic scatterers and the water content in stishovite.
KW - First principles
KW - Hydrous aluminous SiO
KW - Molecular dynamics
KW - Post-stishovite transition
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U2 - 10.1016/j.pepi.2016.03.008
DO - 10.1016/j.pepi.2016.03.008
M3 - Article
AN - SCOPUS:84962788741
SN - 0031-9201
VL - 255
SP - 18
EP - 26
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
ER -