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Phase transition kinetics of superionic H 2 O ice phases revealed by Megahertz X-ray free-electron laser-heating experiments.

Authors :
Husband RJ
Liermann HP
McHardy JD
McWilliams RS
Goncharov AF
Prakapenka VB
Edmund E
Chariton S
Konôpková Z
Strohm C
Sanchez-Valle C
Frost M
Andriambariarijaona L
Appel K
Baehtz C
Ball OB
Briggs R
Buchen J
Cerantola V
Choi J
Coleman AL
Cynn H
Dwivedi A
Graafsma H
Hwang H
Koemets E
Laurus T
Lee Y
Li X
Marquardt H
Mondal A
Nakatsutsumi M
Ninet S
Pace E
Pepin C
Prescher C
Stern S
Sztuk-Dambietz J
Zastrau U
McMahon MI
Source :
Nature communications [Nat Commun] 2024 Sep 23; Vol. 15 (1), pp. 8256. Date of Electronic Publication: 2024 Sep 23.
Publication Year :
2024

Abstract

H <subscript>2</subscript> O transforms to two forms of superionic (SI) ice at high pressures and temperatures, which contain highly mobile protons within a solid oxygen sublattice. Yet the stability field of both phases remains debated. Here, we present the results of an ultrafast X-ray heating study utilizing MHz pulse trains produced by the European X-ray Free Electron Laser to create high temperature states of H <subscript>2</subscript> O, which were probed using X-ray diffraction during dynamic cooling. We confirm an isostructural transition during heating in the 26-69 GPa range, consistent with the formation of SI-bcc. In contrast to prior work, SI-fcc was observed exclusively above ~50 GPa, despite evidence of melting at lower pressures. The absence of SI-fcc in lower pressure runs is attributed to short heating timescales and the pressure-temperature path induced by the pump-probe heating scheme in which H <subscript>2</subscript> O was heated above its melting temperature before the observation of quenched crystalline states, based on the earlier theoretical prediction that SI-bcc nucleates more readily from the fluid than SI-fcc. Our results may have implications for the stability of SI phases in ice-rich planets, for example during dynamic freezing, where the preferential crystallization of SI-bcc may result in distinct physical properties across mantle ice layers.<br /> (© 2024. The Author(s).)

Details

Language :
English
ISSN :
2041-1723
Volume :
15
Issue :
1
Database :
MEDLINE
Journal :
Nature communications
Publication Type :
Academic Journal
Accession number :
39313509
Full Text :
https://doi.org/10.1038/s41467-024-52505-0