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

Abstract:
H2O 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 H2O, 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 H2O 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.
Publication status:
Published
Peer review status:
Peer reviewed

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Author
ORCID:
0000-0002-7666-401X
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Role:
Author
ORCID:
0000-0001-5039-1183
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Author
ORCID:
0000-0002-2630-8092
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ORCID:
0000-0002-3730-8661
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Role:
Author
ORCID:
0000-0002-6422-8819


Publisher:
Nature Research
Journal:
Nature Communications More from this journal
Volume:
15
Issue:
1
Article number:
8256
Publication date:
2024-09-23
Acceptance date:
2024-09-11
DOI:
EISSN:
2041-1723


Language:
English
Pubs id:
2032261
Local pid:
pubs:2032261
Source identifiers:
2280485
Deposit date:
2024-09-23
ARK identifier:
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