Absence of Fermi surface reconstruction in pressure-driven overdoped YBCO
Source abstract
Abstract
The evolution of the critical superconducting temperature and field, quantum oscillation frequencies, and effective mass ${m}*$ in underdoped ${\mathrm{YBa}}2{\mathrm{Cu}}3{\mathrm{O}}_{7\ensuremath{-}\ensuremath{\delta}}$ (YBCO) crystals ($p=0.11$, with $p$ the hole concentration per Cu atom) points to a partial suppression of the charge orders with increasing pressure up to 7 GPa, mimicking doping. Application of pressures up to 25 GPa pushes the sample to the overdoped side of the superconducting dome. In contrast to other cuprates, or to doping studies on YBCO, the frequencies of the quantum oscillations measured in that pressure range do not support the picture of a Fermi-surface reconstruction in the overdoped regime, but possibly point to the existence of a new charge order.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Superconducting Materials and Applications · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
National High Magnetic Field Laboratory
Helmholtz-Zentrum Dresden-Rossendorf
University of British Columbia
Helmut Schmidt University
Brazilian Synchrotron Light Laboratory
Leibniz-Institut für Festkörper- und Werkstoffforschung Dresden
Funding
U.S. Department of Energy · National Nuclear Security Administration · National Science Foundation · State of Florida · Basic Energy Sciences · Deutsche Forschungsgemeinschaft
References (37)
Show source-provided references
1. 10.1103/PhysRevLett.58.90810.1103/PhysRevLett.58.908 ↗
2. 10.1088/0953-8984/21/16/16421210.1088/0953-8984/21/16/164212 ↗
3. 10.1038/nature0633210.1038/nature06332 ↗
4. 10.1103/PhysRevB.83.05450610.1103/PhysRevB.83.054506 ↗
5. 10.1103/PhysRevLett.104.05700510.1103/PhysRevLett.104.057005 ↗
6. 10.1038/nature1034510.1038/nature10345 ↗
7. 10.1038/nphys245610.1038/nphys2456 ↗
8. 10.1126/science.aac625710.1126/science.aac6257 ↗
9. 10.1038/s41535-018-0084-510.1038/s41535-018-0084-5 ↗
10. 10.1038/ncomms311310.1038/ncomms3113 ↗
11. 10.1126/science.aat470810.1126/science.aat4708 ↗
12. 10.1038/nature0587210.1038/nature05872 ↗
13. 10.1038/nature0198110.1038/nature01981 ↗
14. 10.1038/nature0732310.1038/nature07323 ↗
15. 10.1073/pnas.130198911010.1073/pnas.1301989110 ↗
16. 10.1103/PhysRevLett.103.15700210.1103/PhysRevLett.103.157002 ↗
17. 10.1038/ncomms428010.1038/ncomms4280 ↗
18. 10.1103/PhysRevLett.79.529410.1103/PhysRevLett.79.5294 ↗
19. 10.1103/PhysRevB.95.10050510.1103/PhysRevB.95.100505 ↗
20. 10.1103/PhysRevB.56.1416810.1103/PhysRevB.56.14168 ↗
21. 10.1103/PhysRevLett.59.176810.1103/PhysRevLett.59.1768 ↗
22. 10.1103/PhysRevB.47.808910.1103/PhysRevB.47.8089 ↗
23. 10.1080/08957959.2011.63390910.1080/08957959.2011.633909 ↗
24. 10.1021/ac60214a04710.1021/ac60214a047 ↗
25. D. Schoenberg · 2009
26. 10.1063/1.326599210.1063/1.3265992 ↗
27. 10.1103/PhysRevB.61.74110.1103/PhysRevB.61.741 ↗
28. 10.1103/PhysRevB.98.06451310.1103/PhysRevB.98.064513 ↗
29. 10.1073/pnas.221545812010.1073/pnas.2215458120 ↗
30. 10.1038/s41467-017-01465-910.1038/s41467-017-01465-9 ↗
31. 10.1088/0031-8949/44/2/01710.1088/0031-8949/44/2/017 ↗
32. 10.1016/0921-4534(92)90244-710.1016/0921-4534(92)90244-7 ↗
33. 10.1126/science.aaa499010.1126/science.aaa4990 ↗
34. 10.1038/nphys44910.1038/nphys449 ↗
35. 10.1016/S0368-2048(01)00264-X10.1016/S0368-2048(01)00264-X ↗
36. 10.1103/PhysRevLett.95.07700110.1103/PhysRevLett.95.077001 ↗
37. 10.1016/j.crhy.2011.04.01110.1016/j.crhy.2011.04.011 ↗