Underscreened Kondo compensation in a superconductor
Source abstract
Abstract
A magnetic impurity with a larger $S=1$ spin remains partially screened by the Kondo effect when embedded in a metal. However, when placed within an $s$-wave superconductor, the interplay between the superconducting energy gap $Δ$ and the Kondo temperature $T_K$ induces a quantum phase transition from an underscreened doublet Kondo to an unscreened triplet phase, typically occurring when $Δ/T_K\approx 1$. We investigate the Kondo compensation of the impurity spin resulting from this partial screening across the quantum phase transition, which together with the spin-spin correlation function serves as a measure of the Kondo cloud's integrity. Deep within the unscreened triplet phase, $Δ/T_K\gg 1$, the compensation vanishes, signifying complete decoupling of the impurity spin from the environment, while in the partially screened doublet phase, $Δ/T_K\ll 1$, it asymptotically approaches $1/2$, indicating that half of the spin is screened. Notably, there is a universal jump in the compensation precisely at the phase transition, which we accurately calculate. The spin-spin correlation function exhibits an oscillatory pattern with an envelope function decaying as $\sim 1/x$ at short distances. At larger distances, the superconducting gap induces an exponentially decaying behavior $\sim \exp(-x/ξ_Δ)$ governed by the superconducting correlation length $ξ_Δ$, irrespective of the phase, without any distinctive features across the transition. Furthermore, the spectral functions of some relevant operators are evaluated and discussed. In terms of the methods used, a consistent description is provided through the application of multiplicative, numerical and density matrix renormalization group techniques.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Quantum and electron transport phenomena · Numerical methods for differential equations
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Adam Mickiewicz University
Budapest University of Technology and Economics
University of Oradea
Funding
Narodowe Centrum Nauki · Nemzeti Kutatási Fejlesztési és Innovációs Hivatal · Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii
References (61)
Show source-provided references
1. 10.1016/S0031-8914(36)80009-310.1016/S0031-8914(36)80009-3 ↗
2. 10.1143/PTP.32.3710.1143/PTP.32.37 ↗
3. A. C. Hewson · 199310.1017/CBO9780511470752 ↗
4. 10.1038/3437310.1038/34373 ↗
5. 10.1126/science.281.5376.54010.1126/science.281.5376.540 ↗
6. 10.1088/2058-7058/14/1/2810.1088/2058-7058/14/1/28 ↗
7. 10.1051/jphys:0198000410301930010.1051/jphys:01980004103019300 ↗
8. 10.1103/PhysRevB.56.66810.1103/PhysRevB.56.668 ↗
9. 10.1038/3501550910.1038/35015509 ↗
10. 10.1103/PhysRevB.68.22040510.1103/PhysRevB.68.220405 ↗
11. 10.1103/PhysRevLett.94.03680210.1103/PhysRevLett.94.036802 ↗
12. 10.1103/PhysRevB.72.01443010.1103/PhysRevB.72.014430 ↗
13. 10.1021/nn100793s10.1021/nn100793s ↗
14. 10.1103/PhysRevLett.58.92910.1103/PhysRevLett.58.929 ↗
15. 10.1103/PhysRevB.53.915310.1103/PhysRevB.53.9153 ↗
16. 10.1103/PhysRevLett.76.495910.1103/PhysRevLett.76.4959 ↗
17. 10.1103/PhysRevB.75.04130710.1103/PhysRevB.75.041307 ↗
18. 10.1103/PhysRevB.79.10040810.1103/PhysRevB.79.100408 ↗
19. 10.1038/s41586-020-2058-610.1038/s41586-020-2058-6 ↗
20. 10.7498/aps.21.7510.7498/aps.21.75 ↗
21. 10.1143/PTP.40.43510.1143/PTP.40.435 ↗
22. A. I. Rusinov · Sov. Phys. JETP
23. 10.1143/JPSJ.61.323910.1143/JPSJ.61.3239 ↗
24. 10.1038/ncomms998810.1038/ncomms9988 ↗
25. 10.1103/PhysRevB.92.23542210.1103/PhysRevB.92.235422 ↗
26. 10.1103/PhysRevB.95.18050210.1103/PhysRevB.95.180502 ↗
27. 10.1126/science.120220410.1126/science.1202204 ↗
28. 10.1103/PhysRevB.81.12130810.1103/PhysRevB.81.121308 ↗
29. 10.1038/s41567-020-0971-010.1038/s41567-020-0971-0 ↗
30. 10.1103/PhysRevLett.128.24700110.1103/PhysRevLett.128.247001 ↗
31. 10.1103/PhysRevLett.127.18680410.1103/PhysRevLett.127.186804 ↗
32. 10.1103/PhysRevLett.103.19720210.1103/PhysRevLett.103.197202 ↗
33. 10.1103/RevModPhys.47.77310.1103/RevModPhys.47.773 ↗
34. 10.1103/RevModPhys.80.39510.1103/RevModPhys.80.395 ↗
35. 10.1103/PhysRevLett.69.286310.1103/PhysRevLett.69.2863 ↗
36. 10.1103/PhysRevB.48.1034510.1103/PhysRevB.48.10345 ↗
37. 10.1103/RevModPhys.77.25910.1103/RevModPhys.77.259 ↗
38. 10.1016/j.aop.2010.09.01210.1016/j.aop.2010.09.012 ↗
39. 10.1088/0953-8984/19/48/48621110.1088/0953-8984/19/48/486211 ↗
40. 10.1103/PhysRevB.91.04544110.1103/PhysRevB.91.045441 ↗
41. 10.1103/PhysRevB.93.19512510.1103/PhysRevB.93.195125 ↗
42. N. N. Bogoliubov · Sov. Phys. JETP
43. 10.1103/RevModPhys.45.58910.1103/RevModPhys.45.589 ↗
44. 10.1007/BF0011796310.1007/BF00117963 ↗
45. 10.1103/PhysRevB.57.43210.1103/PhysRevB.57.432 ↗
46. 10.1088/1742-5468/2007/01/L0100110.1088/1742-5468/2007/01/L01001 ↗
47. 10.1103/PhysRevB.77.10440110.1103/PhysRevB.77.104401 ↗
48. 10.1103/PhysRevB.80.20511410.1103/PhysRevB.80.205114 ↗
49. 10.1103/PhysRevB.81.04511110.1103/PhysRevB.81.045111 ↗
50. 10.1103/PhysRevB.84.11512010.1103/PhysRevB.84.115120 ↗
51. 10.1103/PhysRevB.88.09430610.1103/PhysRevB.88.094306 ↗
52. 10.1103/PhysRevB.90.04511710.1103/PhysRevB.90.045117 ↗
53. 10.1103/PhysRevB.89.10410210.1103/PhysRevB.89.104102 ↗
54. 10.1103/PhysRevB.106.12511510.1103/PhysRevB.106.125115 ↗
55. 10.1038/s41467-023-39234-610.1038/s41467-023-39234-6 ↗
56. 10.1103/PhysRevB.95.08511510.1103/PhysRevB.95.085115 ↗
57. 10.1103/PhysRevB.97.15515610.1103/PhysRevB.97.155156 ↗
58. 10.5281/zenodo.1451277710.5281/zenodo.14512777 ↗
59. 10.1103/PhysRevB.21.100310.1103/PhysRevB.21.1003 ↗
60. 10.21468/SciPostPhysCodeb.410.21468/SciPostPhysCodeb.4 ↗
61. 10.21468/SciPostPhysCodeb.4-r0.310.21468/SciPostPhysCodeb.4-r0.3 ↗