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@ARTICLE{Husband:612515,
author = {Husband, Rachel and Liermann, Hanns-Peter and McHardy,
James and Mcwilliams, Ryan Stewart and Goncharov, Alexander
and Prakapenka, Vitali and Edmund, Eric and Chariton, Stella
and Konopkova, Zuzana and Strohm, Cornelius and
Sanchez-Valle, Carmen and Frost, Mungo and
Andriambariarijaona, Leon and Appel, Karen and Baehtz,
Carsten and Ball, Orianna and Briggs, Richard and Buchen,
Johannes and Cerantola, Valerio and Choi, Jinhyuk and
Coleman, Amy and CYNN, HYUNCHAE and Dwivedi, Anand and
Graafsma, Heinz and Hwang, Huijeong and Koemets, Egor and
Laurus, Torsten and Lee, Yongjae and Li, Xinyang and
Marquardt, Hauke and Mondal, Anshuman and Nakatsutsumi,
Motoaki and NINET, Sandra and Pace, Edward and Pépin,
Charles and Prescher, Clemens and Stern, Stephan and
Sztuk-Dambietz, Jolanta and Zastrau, Ulf and McMahon,
Malcolm},
title = {{P}hase transition kinetics of superionic ${H}_2{O}$ ice
phases revealed by {MH}z {XFEL} heating experiments},
journal = {Nature Communications},
volume = {15},
number = {1},
issn = {2041-1723},
address = {[London]},
publisher = {Nature Publishing Group UK},
reportid = {PUBDB-2024-05368},
pages = {8256},
year = {2024},
note = {We acknowledge support from the Deutsche
For-schungsgemeinschaft (DFG) Research Unit FOR 2440 grants
SA2585/5-1 (R.J.H, A.M., C.S.V., and H.P.L) and AP262/2-2
(K.A.).},
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 these 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.},
cin = {FS-HIBEF / XFEL-User / $XFEL_E1_HED$ / FS-DS / DOOR ;
HAS-User / FS-PET-D},
ddc = {500},
cid = {I:(DE-H253)FS-HIBEF-20240110 /
I:(DE-H253)XFEL-User-20170713 /
$I:(DE-H253)XFEL_E1_HED-20210408$ /
I:(DE-H253)FS-DS-20120731 / I:(DE-H253)HAS-User-20120731 /
I:(DE-H253)FS-PET-D-20190712},
pnm = {631 - Matter – Dynamics, Mechanisms and Control
(POF4-631) / 6G3 - PETRA III (DESY) (POF4-6G3) / DFG project
280637173 - FOR 2440: Materie im Inneren von Planeten -
Hochdruck-, Planeten- und Plasmaphysik (280637173)},
pid = {G:(DE-HGF)POF4-631 / G:(DE-HGF)POF4-6G3 /
G:(GEPRIS)280637173},
experiment = {EXP:(DE-H253)XFEL-HED-20150101 /
EXP:(DE-H253)P-P02.2-20150101},
typ = {PUB:(DE-HGF)16},
pubmed = {pmid:39313509},
UT = {WOS:001320768800004},
doi = {10.1038/s41467-024-52505-0},
url = {https://bib-pubdb1.desy.de/record/612515},
}