High-temperature superconductivity in La4H23 below 100 GPa
Source abstract
Abstract
High-temperature superconductivity has been observed in binary hydrides such as {LaH}10 at pressures close to 180 GPa, whereby hydrogen cagelike structures have been identified as a common motif beneficial for high critical temperatures {T}c. Efforts are now focused on finding hydride high-temperature superconductors at lower pressures. We present evidence for high-temperature superconductivity in binary {La}4{H}23 at a pressure of P=95 GPa, with A15-type arrangement of the lanthanum atoms in the type-I clathrate structure. We synthesize {La}4{H}23 from a lanthanum film capped with a palladium catalyst promoting the dissociation of hydrogen. In resistance measurements, we observe superconductivity with a transition temperature {T}c∼90 K. The A15-type lanthanum sublattice is identified in x-ray diffraction on the same sample, in agreement with previous x-ray diffraction and structure prediction studies. Our study reinforces the favorability of cagelike networks of the hydrogen lattice for high-temperature superconductivity. Published by the American Physical Society 2024
Source: crossref · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: High-pressure geophysics and materials · Rare-earth and actinide compounds · Advanced Chemical Physics Studies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
HH Wills Laboratory, University of Bristol, Bristol BS8 1TL, United Kingdom
Diamond Light Source, Chilton, Oxfordshire OX11 0DE, United Kingdom
Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, United Kingdom
Funding
European Research Council · Engineering and Physical Sciences Research Council
References (27)
Show source-provided references
1. 10.1103/PhysRevLett.122.02700110.1103/PhysRevLett.122.027001 ↗
2. 10.1038/s41586-019-1201-810.1038/s41586-019-1201-8 ↗
3. 10.1038/s41467-021-25372-210.1038/s41467-021-25372-2 ↗
4. 10.1146/annurev-conmatphys-031218-01341310.1146/annurev-conmatphys-031218-013413 ↗
5. 10.1038/s41467-023-38254-610.1038/s41467-023-38254-6 ↗
6. 10.1038/s41467-022-34755-y10.1038/s41467-022-34755-y ↗
7. 10.1021/acs.jpclett.1c0082610.1021/acs.jpclett.1c00826 ↗
8. 10.1103/PhysRevB.96.10050210.1103/PhysRevB.96.100502 ↗
9. 10.1016/j.physrep.2020.02.00310.1016/j.physrep.2020.02.003 ↗
10. 10.1007/s11433-023-2101-910.1007/s11433-023-2101-9 ↗
11. 10.1021/acs.jpclett.0c0333110.1021/acs.jpclett.0c03331 ↗
12. 10.1103/PhysRevLett.126.11700310.1103/PhysRevLett.126.117003 ↗
13. 10.1103/PhysRevB.106.13450910.1103/PhysRevB.106.134509 ↗
14. 10.1107/S002188980801201610.1107/S0021889808012016 ↗
15. 10.1038/nature1496410.1038/nature14964 ↗
16. 10.1038/s41586-020-1955-z10.1038/s41586-020-1955-z ↗
17. 10.1038/nature1717510.1038/nature17175 ↗
18. 10.1088/0953-2048/27/1/01500510.1088/0953-2048/27/1/015005 ↗
19. 10.1103/PhysRevB.105.L22050210.1103/PhysRevB.105.L220502 ↗
20. 10.1063/1.233568310.1063/1.2335683 ↗
21. 10.1103/PhysRevB.102.13451010.1103/PhysRevB.102.134510 ↗
22. 10.1103/PhysRevB.78.10411910.1103/PhysRevB.78.104119 ↗
23. 10.1016/j.pepi.2014.05.00510.1016/j.pepi.2014.05.005 ↗
24. 10.1080/08957959.2015.105983510.1080/08957959.2015.1059835 ↗
25. 10.1107/S002188981300353110.1107/S0021889813003531 ↗
26. 10.1107/S160057751500228310.1107/S1600577515002283 ↗
27. 10.5523/bris.22buhfhub62xs2c7xv5w0pa10d10.5523/bris.22buhfhub62xs2c7xv5w0pa10d ↗