journal article·2025-07-23Open access

Structure factors and quantum geometry in multiband BCS superconductors

M. Iskin

Physical Review B· Volume 112· Issue 1

Abstract

We consider multiband BCS superconductors that exhibit time-reversal symmetry and uniform pairing, and analyze their dynamic density and spin structure factors using linear-response theory within the mean-field BCS-BEC crossover framework at zero temperature. Our results for the multi-orbital Hubbard model satisfy the associated f-sum rules in several limits. In particular, in the strong-coupling limit, they coincide with those of a weakly-interacting Bose gas of Cooper pairs, where the low-energy collective Goldstone modes serve as Bogoliubov phonons. We further reveal that the quantum-geometric origin of the low-energy structure factors, along with related observables such as the superfluid-weight tensor and the effective-mass tensor of Cooper pairs, can be traced all the way back to the effective-mass theorem for Bloch bands in this limit. As an illustration, we investigate the pyrochlore-Hubbard model numerically and demonstrate that the Goldstone modes are the only relevant collective degrees of freedom in the flat-band regime.
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Research context

OpenAlex topics: Superconductivity in MgB2 and Alloys · Physics of Superconductivity and Magnetism · Iron-based superconductors research

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Koç University

Funding

Air Force Office of Scientific Research

References (46)

Show source-provided references
1. 10.1103/PhysRevLett.122.21040110.1103/PhysRevLett.122.210401 ↗
2. 10.1093/nsr/nwz19310.1093/nsr/nwz193 ↗
3. 10.1038/s41586-020-1989-210.1038/s41586-020-1989-2 ↗
4. 10.1038/s41586-022-05576-210.1038/s41586-022-05576-2 ↗
5. 10.1103/PhysRevResearch.5.L03201610.1103/PhysRevResearch.5.L032016 ↗
6. 10.1126/science.adf150610.1126/science.adf1506 ↗
7. 10.1126/science.ado604910.1126/science.ado6049 ↗
8. 10.1038/s41567-024-02678-810.1038/s41567-024-02678-8 ↗
9. 10.1007/BF0219355910.1007/BF02193559 ↗
10. 10.1098/rspa.1984.002310.1098/rspa.1984.0023 ↗
11. 10.1140/epjb/e2010-10874-410.1140/epjb/e2010-10874-4 ↗
12. 10.1038/s42254-022-00466-y10.1038/s42254-022-00466-y ↗
13. 10.1103/PhysRevLett.131.24000110.1103/PhysRevLett.131.240001 ↗
14. 10.1088/1361-6633/ade45410.1088/1361-6633/ade454 ↗
15. 10.1103/PhysRevLett.133.20660210.1103/PhysRevLett.133.206602 ↗
16. D. Pines · 1966
17. 10.1209/epl/i2006-10165-x10.1209/epl/i2006-10165-x ↗
18. 10.1016/j.aop.2016.07.03010.1016/j.aop.2016.07.030 ↗
19. 10.1007/s10909-012-0853-710.1007/s10909-012-0853-7 ↗
20. 10.1103/PhysRevLett.132.03600110.1103/PhysRevLett.132.036001 ↗
21. 10.1103/PhysRevA.99.05360310.1103/PhysRevA.99.053603 ↗
22. 10.1103/PhysRevX.14.01105210.1103/PhysRevX.14.011052 ↗
23. 10.1103/PhysRevB.95.02451510.1103/PhysRevB.95.024515 ↗
24. 10.1103/PhysRevB.109.17450810.1103/PhysRevB.109.174508 ↗
25. 10.1007/BF0068377410.1007/BF00683774 ↗
26. 10.1103/PhysRevA.97.01361810.1103/PhysRevA.97.013618 ↗
27. A. Leggett · 2008
28. 10.1103/PhysRevB.111.01450210.1103/PhysRevB.111.014502 ↗
29. 10.1103/PhysRevB.55.1515310.1103/PhysRevB.55.15153 ↗
30. 10.1103/PhysRevB.110.14450510.1103/PhysRevB.110.144505 ↗
31. 10.1103/PhysRevLett.132.02600210.1103/PhysRevLett.132.026002 ↗
32. 10.1103/PhysRevB.107.22450510.1103/PhysRevB.107.224505 ↗
33. 10.1103/PhysRevLett.93.08040110.1103/PhysRevLett.93.080401 ↗
34. 10.1103/PhysRevA.94.06361810.1103/PhysRevA.94.063618 ↗
35. 10.1103/PhysRevB.45.316410.1103/PhysRevB.45.3164 ↗
36. 10.1103/PhysRevB.47.625610.1103/PhysRevB.47.6256 ↗
37. 10.1038/s41586-023-06640-110.1038/s41586-023-06640-1 ↗
38. 10.1038/s41535-024-00683-x10.1038/s41535-024-00683-x ↗
39. 10.1088/1367-2630/18/11/11304410.1088/1367-2630/18/11/113044 ↗
40. 10.1038/nphys418710.1038/nphys4187 ↗
41. 10.1103/PhysRevLett.128.10040110.1103/PhysRevLett.128.100401 ↗
42. 10.1103/PhysRevB.49.682910.1103/PhysRevB.49.6829 ↗
43. 10.1103/PhysRevB.103.L04130310.1103/PhysRevB.103.L041303 ↗
44. 10.1103/PhysRevResearch.4.02311210.1103/PhysRevResearch.4.023112 ↗
45. 10.1103/PhysRevLett.122.09340310.1103/PhysRevLett.122.093403 ↗
46. 10.1103/PhysRevA.105.02331210.1103/PhysRevA.105.023312 ↗