journal article·2020-05-13Open access

Pairing instability on a Luttinger surface: A non-Fermi liquid to superconductor transition and its Sachdev-Ye-Kitaev dual

Chandan Setty

Physical Review B· Volume 101· Issue 18

Abstract

Superconductivity results from an instability of the Fermi surface---contour of poles of the single-particle propagator---to an infinitesimally small attraction between electrons. Here, we instead discuss the analogous problem on a model Luttinger surface, or contour of zeros of the Green function. At zero temperature $(\ensuremath{\beta}\ensuremath{\rightarrow}\ensuremath{\infty})$ and a critical interaction strength $({u}_{c\ensuremath{\infty}})$ characterized by the residue of self-energy pole, we find that the pair susceptibility diverges leading to a superconducting instability. We evaluate the pair fluctuation partition function and find that the spectral density in the normal state has an interaction-driven, power-law $\frac{1}{\sqrt{\ensuremath{\omega}}}$ type, van-Hove singularity (vHS), indicating non-Fermi liquid (NFL) physics. Crucially, in the strong coupling limit $(\ensuremath{\beta}u\ensuremath{\gg}1)$, the leading-order fluctuation free-energy terms in the normal state of this NFL-SC transition resembles the equivalent $\left[O(1)\right]$ terms of the Sachdev-Ye-Kitaev (SYK) model. This free-energy contribution takes a simple form $\ensuremath{-}\ensuremath{\beta}F=\ensuremath{\beta}{u}_{c\ensuremath{\infty}}\ensuremath{-}\ensuremath{\gamma}\phantom{\rule{0.16em}{0ex}}\text{ln}\left(\ensuremath{\beta}{u}_{c\ensuremath{\infty}}\right),$ where $\ensuremath{\gamma}$ is a constant equal to $\frac{1}{2}$. Weak impurity scattering $(\ensuremath{\tau}\ensuremath{\gg}{\ensuremath{\beta}}^{\ensuremath{-}1})$ leaves the low-energy spectral density unaffected but leads to an interaction-driven enhancement of superconductivity. Our results shed light on the role played by order-parameter fluctuations in providing the key missing link between Mott physics and strongly coupled toy models exhibiting gravity duals.
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Research context

OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics · Iron-based superconductors research

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References (56)

Show source-provided references
1. A. A. Abrikosov · 1965
2. 10.1088/0034-4885/62/1/00210.1088/0034-4885/62/1/002 ↗
3. 10.1103/PhysRevB.74.22451010.1103/PhysRevB.74.224510 ↗
4. 10.1088/1367-2630/12/10/10500810.1088/1367-2630/12/10/105008 ↗
5. 10.1088/1367-2630/13/1/01303110.1088/1367-2630/13/1/013031 ↗
6. 10.1103/PhysRevLett.107.04700310.1103/PhysRevLett.107.047003 ↗
7. 10.1088/0034-4885/74/2/02250110.1088/0034-4885/74/2/022501 ↗
8. 10.1103/PhysRev.119.115310.1103/PhysRev.119.1153 ↗
9. 10.1103/PhysRev.118.141710.1103/PhysRev.118.1417 ↗
10. 10.1103/PhysRevLett.84.337010.1103/PhysRevLett.84.3370 ↗
11. 10.1051/jp1:199612710.1051/jp1:1996127 ↗
12. 10.1103/PhysRevB.68.08511310.1103/PhysRevB.68.085113 ↗
13. 10.1103/PhysRevB.65.11511710.1103/PhysRevB.65.115117 ↗
14. 10.1103/PhysRevLett.96.08640710.1103/PhysRevLett.96.086407 ↗
15. 10.1103/PhysRevB.73.17450110.1103/PhysRevB.73.174501 ↗
16. 10.1209/epl/i1998-00164-y10.1209/epl/i1998-00164-y ↗
17. 10.1103/PhysRevB.74.12511010.1103/PhysRevB.74.125110 ↗
18. 10.1103/PhysRevB.75.10450310.1103/PhysRevB.75.104503 ↗
19. 10.1140/epjb/e2007-00312-310.1140/epjb/e2007-00312-3 ↗
20. 10.1103/PhysRevLett.110.09040310.1103/PhysRevLett.110.090403 ↗
21. 10.1103/PhysRevLett.97.13640110.1103/PhysRevLett.97.136401 ↗
22. 10.1103/PhysRevLett.102.05640410.1103/PhysRevLett.102.056404 ↗
23. 10.1016/j.aop.2006.04.00310.1016/j.aop.2006.04.003 ↗
24. 10.1103/PhysRevLett.98.22700210.1103/PhysRevLett.98.227002 ↗
25. 10.1103/PhysRevB.76.17450110.1103/PhysRevB.76.174501 ↗
26. 10.1007/JHEP09(2018)00910.1007/JHEP09(2018)009 ↗
27. 10.1073/pnas.172058011510.1073/pnas.1720580115 ↗
28. 10.1103/PhysRevB.86.11511810.1103/PhysRevB.86.115118 ↗
29. 10.1103/PhysRevLett.79.110610.1103/PhysRevLett.79.1106 ↗
30. 10.1103/PhysRevLett.79.111010.1103/PhysRevLett.79.1110 ↗
31. 10.1103/PhysRevB.96.08512410.1103/PhysRevB.96.085124 ↗
32. 10.1103/PhysRevB.63.13440610.1103/PhysRevB.63.134406 ↗
34. 10.1103/RevModPhys.90.01500910.1103/RevModPhys.90.015009 ↗
35. 10.1103/PhysRevB.44.954110.1103/PhysRevB.44.9541 ↗
36. 10.1103/PhysRevB.55.R1474510.1103/PhysRevB.55.R14745 ↗
37. 10.1016/0921-4534(93)90981-U10.1016/0921-4534(93)90981-U ↗
38. 10.1007/BF0065554610.1007/BF00655546 ↗
39. 10.1103/PhysRevB.72.06452310.1103/PhysRevB.72.064523 ↗
40. 10.1103/PhysRevD.94.10600210.1103/PhysRevD.94.106002 ↗
41. 10.1007/JHEP05(2017)11810.1007/JHEP05(2017)118 ↗
42. 10.1103/PhysRevB.83.20513710.1103/PhysRevB.83.205137 ↗
43. 10.1103/PhysRevLett.106.09160210.1103/PhysRevLett.106.091602 ↗
44. 10.1103/PhysRevD.83.04601210.1103/PhysRevD.83.046012 ↗
45. 10.1098/rsta.2015.024810.1098/rsta.2015.0248 ↗
46. 10.1103/PhysRevLett.90.21640310.1103/PhysRevLett.90.216403 ↗
47. 10.1103/PhysRevB.85.13451910.1103/PhysRevB.85.134519 ↗
48. 10.1103/PhysRevB.85.19512310.1103/PhysRevB.85.195123 ↗
49. 10.1103/PhysRevB.100.11513210.1103/PhysRevB.100.115132 ↗
50. 10.1103/PhysRevLett.70.333910.1103/PhysRevLett.70.3339 ↗
51. 10.1103/PhysRevLett.105.15160210.1103/PhysRevLett.105.151602 ↗
52. 10.1103/PhysRevB.95.15513110.1103/PhysRevB.95.155131 ↗
53. 10.1143/PTP.94.18110.1143/PTP.94.181 ↗
54. 10.1103/PhysRevB.66.06452610.1103/PhysRevB.66.064526 ↗
55. 10.1103/PhysRevB.99.14452310.1103/PhysRevB.99.144523 ↗
56. 10.1143/JPSJ.61.205610.1143/JPSJ.61.2056 ↗