TY - JOUR
T1 - Effect of nickel on the high-pressure phases in FeH
AU - Piet, Helene
AU - Chizmeshya, Andrew V.G.
AU - Chen, Bin
AU - Chariton, Stella
AU - Greenberg, Eran
AU - Prakapenka, Vitali B.
AU - Shim, Sang Heon
N1 - Funding Information:
The work has been supported by the NASA (80NSSC18K0353) and NSF (EAR1921298 and AST2005567). H.P. and S.-H.S. were supported partially by the Keck Foundation (PI: P. Buseck). The results reported herein benefit from collaborations and information exchange within NASA's Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA's Science Mission Directorate. A.V.G.C. gratefully acknowledges ASU's supercomputing resources. B.C. acknowledges the support from NSF (EAR-1555388, EAR-1829273). The synchrotron experiments were conducted at GeoSoilEnviroCARS (University of Chicago, Sector 13), Advanced Photon Source (APS). GeoSoilEnviroCARS is supported by the NSF-Earth Science (EAR-1634415) and DOE-GeoScience (DE-FG02-94ER14466). A.P.S. is supported by DOE-BES under contract DE-AC02-06CH11357.
Publisher Copyright:
© 2021 American Physical Society
PY - 2021/12/1
Y1 - 2021/12/1
N2 - Hydrogen-rich metal alloys and compounds have drawn interest from planetary geophysics and condensed matter physics communities because of their potential for deep hydrogen storage in planets and high-temperature superconductivity. We find that a small amount of Ni can alter the phase behavior in the FeH alloy system. Ni can stabilize the double hexagonal close-packed (dhcp) structure in FeH up to the liquidus at 33 GPa, which is in contrast with the stability of the face-centered cubic (fcc) structure in Ni-free FeH at the same conditions. Above 60 GPa, Ni suppresses the stability of the tetragonal FeH2 phase but stabilizes fcc FeH at higher temperatures. At the same pressure range, we find tetragonal FeH2 and cubic FeH3 to be stable at temperatures above 2500 K without Ni. Therefore, in planetary interiors, Ni will expand the stability field of dense close-packed structures in the FeH system. If the Ni content is low, then FeH2 and FeH3 can play an important role in the cores of hydrogen-rich planets. Also, our study demonstrates that a secondary alloying component can severely impact the high-pressure stability of polyhydrides.
AB - Hydrogen-rich metal alloys and compounds have drawn interest from planetary geophysics and condensed matter physics communities because of their potential for deep hydrogen storage in planets and high-temperature superconductivity. We find that a small amount of Ni can alter the phase behavior in the FeH alloy system. Ni can stabilize the double hexagonal close-packed (dhcp) structure in FeH up to the liquidus at 33 GPa, which is in contrast with the stability of the face-centered cubic (fcc) structure in Ni-free FeH at the same conditions. Above 60 GPa, Ni suppresses the stability of the tetragonal FeH2 phase but stabilizes fcc FeH at higher temperatures. At the same pressure range, we find tetragonal FeH2 and cubic FeH3 to be stable at temperatures above 2500 K without Ni. Therefore, in planetary interiors, Ni will expand the stability field of dense close-packed structures in the FeH system. If the Ni content is low, then FeH2 and FeH3 can play an important role in the cores of hydrogen-rich planets. Also, our study demonstrates that a secondary alloying component can severely impact the high-pressure stability of polyhydrides.
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U2 - 10.1103/PhysRevB.104.224106
DO - 10.1103/PhysRevB.104.224106
M3 - Article
AN - SCOPUS:85122073863
SN - 2469-9950
VL - 104
JO - Physical Review B
JF - Physical Review B
IS - 22
M1 - 224106
ER -