Doping dependence of the low-temperature planar carrier density in overdoped YBa 2 Cu 3 O 7 − δ
Source abstract
Abstract
Whether a quantum critical point (QCP) demarcates the end of the pseudogap (PG) regime in hole-doped cuprates at a singular doping level {p}*≈0.19 is still an open question. A crucial component of the puzzle is the manner in which the carrier density predicted by electronic structure calculations is recovered for p>{p}* . Here, we use magnetic fields up to 67 T to suppress superconductivity down to 50 K, allowing us to simultaneously measure the low-temperature Hall number {n}H and the in-plane resistivity anisotropy {ρ}a/{ρ}b in overdoped {Y}1−x{Ca}x{Ba}2{Cu}3{O}7−δ single crystals. We confirm a previous finding [S. Badoux , ] that {n}H (50 K) exhibits a sharp increase below {p}* and use the measured resistivity anisotropy to obtain the planar carrier density {n}pl={n}H{({ρ}a/{ρ}b)}−1 . The doping dependence of {n}pl (50 K) reveals two key findings: (i) At optimal doping, {n}pl≈p , and (ii) the sharp rise in {n}H(p) is softened to such an extent that the full Fermi volume ( {n}pl=1+p ) is only partially recovered at {p}* . The latter result disfavors a conventional QCP scenario in which the PG end point leads to a reconstructed Fermi surface.
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Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Magnetic properties of thin films · Theoretical and Computational Physics
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
University of Bristol
Helmholtz-Zentrum Dresden-Rossendorf
Radboud University
Funding
Horizon 2020 · Engineering and Physical Sciences Research Council
References (65)
Show source-provided references
1. 10.1038/nature1416510.1038/nature14165 ↗
2. 10.1103/PhysRevLett.89.14700310.1103/PhysRevLett.89.147003 ↗
3. 10.1103/PhysRevB.68.10050210.1103/PhysRevB.68.100502 ↗
4. 10.1088/1367-2630/12/10/10500910.1088/1367-2630/12/10/105009 ↗
5. 10.1103/PhysRevLett.69.285510.1103/PhysRevLett.69.2855 ↗
6. 10.1103/PhysRevB.77.22050210.1103/PhysRevB.77.220502 ↗
7. 10.1038/nature0189010.1038/nature01890 ↗
8. 10.1038/nature0633210.1038/nature06332 ↗
9. 10.1038/s41567-021-01197-010.1038/s41567-021-01197-0 ↗
10. 10.1038/nature1698310.1038/nature16983 ↗
11. 10.1209/0295-5075/113/2700310.1209/0295-5075/113/27003 ↗
12. 10.1103/PhysRevB.111.06451810.1103/PhysRevB.111.064518 ↗
13. 10.1103/PhysRevB.95.22451710.1103/PhysRevB.95.224517 ↗
14. 10.1038/s41586-019-0932-x10.1038/s41586-019-0932-x ↗
15. 10.1103/PhysRevB.106.19511010.1103/PhysRevB.106.195110 ↗
16. 10.1126/science.116501510.1126/science.1165015 ↗
17. 10.1088/1742-6596/449/1/01200410.1088/1742-6596/449/1/012004 ↗
18. 10.1088/1361-6633/aaa97c10.1088/1361-6633/aaa97c ↗
19. 10.1126/science.aan317810.1126/science.aan3178 ↗
20. 10.1038/s41586-021-03622-z10.1038/s41586-021-03622-z ↗
21. 10.1038/s41467-024-52564-310.1038/s41467-024-52564-3 ↗
22. 10.1103/PhysRevB.69.10452110.1103/PhysRevB.69.104521 ↗
23. 10.1103/PhysRevB.43.19310.1103/PhysRevB.43.193 ↗
24. 10.1103/PhysRevLett.88.13700510.1103/PhysRevLett.88.137005 ↗
25. 10.21468/SciPostPhys.11.1.01210.21468/SciPostPhys.11.1.012 ↗
26. 10.1103/PhysRevB.73.18050510.1103/PhysRevB.73.180505 ↗
27. 10.1080/14786435.2012.66906510.1080/14786435.2012.669065 ↗
28. 10.1063/1.166065610.1063/1.1660656 ↗
29. 10.1063/1.365290510.1063/1.3652905 ↗
30. 10.1103/PhysRevLett.70.399510.1103/PhysRevLett.70.3995 ↗
31. 10.1103/PhysRevB.60.R1503510.1103/PhysRevB.60.R15035 ↗
32. 10.1103/PhysRevLett.99.02700310.1103/PhysRevLett.99.027003 ↗
33. 10.1103/PhysRevLett.113.17700510.1103/PhysRevLett.113.177005 ↗
34. 10.1073/pnas.160270911310.1073/pnas.1602709113 ↗
35. 10.1103/PhysRevMaterials.6.04480410.1103/PhysRevMaterials.6.044804 ↗
36. 10.1063/1.10327910.1063/1.103279 ↗
37. 10.1016/j.jallcom.2015.11.01910.1016/j.jallcom.2015.11.019 ↗
38. 10.1143/JJAP.34.475410.1143/JJAP.34.4754 ↗
39. 10.1103/PhysRevB.47.605410.1103/PhysRevB.47.6054 ↗
40. 10.1002/pssa.221102024910.1002/pssa.2211020249 ↗
41. 10.1126/science.aaa499010.1126/science.aaa4990 ↗
42. 10.1016/j.phpro.2012.04.08110.1016/j.phpro.2012.04.081 ↗
43. 10.1103/PhysRev.140.A186910.1103/PhysRev.140.A1869 ↗
44. 10.1103/PhysRevLett.57.62610.1103/PhysRevLett.57.626 ↗
45. 10.1103/PhysRevLett.111.16700110.1103/PhysRevLett.111.167001 ↗
46. 10.1103/PhysRevLett.110.25700210.1103/PhysRevLett.110.257002 ↗
47. 10.1016/0921-4534(95)00770-910.1016/0921-4534(95)00770-9 ↗
48. 10.1103/PhysRevLett.71.174010.1103/PhysRevLett.71.1740 ↗
49. 10.1016/0022-3697(95)00269-310.1016/0022-3697(95)00269-3 ↗
50. 10.1103/PhysRevB.76.14050810.1103/PhysRevB.76.140508 ↗
51. 10.1016/0921-4534(94)90768-410.1016/0921-4534(94)90768-4 ↗
52. 10.1126/science.121982110.1126/science.1219821 ↗
53. 10.1038/s41467-022-28124-y10.1038/s41467-022-28124-y ↗
54. 10.1103/PhysRevLett.102.01700410.1103/PhysRevLett.102.017004 ↗
55. 10.1038/nphys165610.1038/nphys1656 ↗
56. 10.1038/s41567-020-0982-x10.1038/s41567-020-0982-x ↗
57. 10.1103/PhysRevResearch.3.02306910.1103/PhysRevResearch.3.023069 ↗
58. 10.1073/pnas.100920210710.1073/pnas.1009202107 ↗
59. 10.1038/s41567-024-02564-310.1038/s41567-024-02564-3 ↗
60. 10.1103/PhysRev.79.191.210.1103/PhysRev.79.191.2 ↗
61. 10.1088/0370-1298/65/6/11410.1088/0370-1298/65/6/114 ↗
62. 10.5523/bris.1645z6yvvvb9d2gznuchw70nnc10.5523/bris.1645z6yvvvb9d2gznuchw70nnc ↗
63. 10.1007/s10948-022-06183-y10.1007/s10948-022-06183-y ↗
64. 10.1038/s41563-023-01497-110.1038/s41563-023-01497-1 ↗
65. 10.1038/s41467-024-49325-710.1038/s41467-024-49325-7 ↗