Author Affiliations
Abstract
1 Center for High Pressure Science and Technology Advanced Research, Beijing 100094, China
2 High Pressure Collaborative Access Team, Geophysical Laboratory, Carnegie Institution of Washington, Argonne, Illinois 60439, USA
3 Center for the Study of Matter at Extreme Conditions and Department of Mechanical and Materials Engineering, Florida International University, Miami, Florida 33199, USA
4 Advanced Photon Source, Argonne National Laboratory, Lemont, Illinois 60439, USA
5 HPCAT, X-Ray Science Division, Argonne National Laboratory, Lemont, Illinois 60439, USA
6 MAX IV Laboratory, Lund University, 22100 Lund, Sweden
7 Condensed Matter Theory Group, Materials Theory Division, Department of Physics and Astronomy, Uppsala University, Uppsala S-75120, Sweden
8 Center for Advanced Radiation Sources, University of Chicago, Chicago, Illinois 60637, USA
9 Department of Engineering Sciences and Mathematics, Luleå University of Technology, 97187 Luleå, Sweden
Diamond anvil cell techniques have been improved to allow access to the multimegabar ultrahigh-pressure region for exploring novel phenomena in condensed matter. However, the only way to determine crystal structures of materials above 100 GPa, namely, X-ray diffraction (XRD), especially for low Z materials, remains nontrivial in the ultrahigh-pressure region, even with the availability of brilliant synchrotron X-ray sources. In this work, we perform a systematic study, choosing hydrogen (the lowest X-ray scatterer) as the subject, to understand how to better perform XRD measurements of low Z materials at multimegabar pressures. The techniques that we have developed have been proved to be effective in measuring the crystal structure of solid hydrogen up to 254 GPa at room temperature [C. Ji et al., Nature 573, 558–562 (2019)]. We present our discoveries and experiences with regard to several aspects of this work, namely, diamond anvil selection, sample configuration for ultrahigh-pressure XRD studies, XRD diagnostics for low Z materials, and related issues in data interpretation and pressure calibration. We believe that these methods can be readily extended to other low Z materials and can pave the way for studying the crystal structure of hydrogen at higher pressures, eventually testing structural models of metallic hydrogen.
Matter and Radiation at Extremes
2020, 5(3): 038401
Author Affiliations
Abstract
1 Center for High Pressure Science and Technology Advanced Research, Shanghai, China
2 Center for High Pressure Science and Technology Advanced Research, Shanghai, China
3 Center for Advanced Radiation Sources, The University of Chicago, 5640 South Ellis Avenue, Chicago, Illinois 60637, USA
4 Federal Scientific Research Center Crystallography and Photonics, Russian Academy of Sciences, 59 Leninskii Pr-t, Moscow 119333, Russia
5 Federal Scientific Research Center Crystallography and Photonics, Russian Academy of Sciences, 59 Leninskii Pr-t, Moscow 119333, Russia
Recent reports of the superconductivity in hydrides of two different families (covalent lattice, as in SH3 and clathrate-type H-cages containing La and Y atoms, as in LaH10 and YH6) have revealed new families of high-Tc materials with Tc’s near room temperature values. These findings confirm earlier expectations that hydrides may have very high Tc’s due to the fact that light H atoms have very high vibrational frequencies, leading to high Tc values within the conventional Bardeen–Cooper–Schrieffer phonon mechanism of superconductivity. However, as is pointed out by Ashcroft, it is important to have the metallic hydrogen “alloyed” with the elements added to it. This concept of a metallic alloy containing a high concentration of metal-like hydrogen atoms has been instrumental in finding new high-Tc superhydrides. These new superhydride “room-temperature” superconductors are stabilized only at very high pressures above 100 GPa, making the experimental search for their superconducting properties very difficult. We will review the current experimental and theoretical results for LaH10?x and YH6?x superhydrides.
Matter and Radiation at Extremes
2020, 5(2): 028201

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