Spin-phonon interactions on the kagome lattice: Dirac spin liquid versus valence-bond solids
Source abstract
Abstract
We investigate the impact of spin-phonon coupling on the $S=1/2$ Heisenberg model on the kagome lattice. For the pure spin model, there is increasing evidence that the low-energy properties can be correctly described by a Dirac spin liquid, in which spinons with a conical dispersion are coupled to emergent gauge fields. Within this scenario, the ground-state wave function is well approximated by a Gutzwiller-projected fermionic state [Ran, Hermele, Lee, and Wen, Phys. Rev. Lett. 98, 117205 (2007)]. However, the existence of $U(1)$ gauge fields may naturally lead to instabilities when small perturbations are included. Phonons are ubiquitous in real materials and may play a relevant role in the determination of the actual physical properties of the kagome antiferromagnet. Therefore, we perform a step forward in this direction, including phonon degrees of freedom (at the quantum level) and applying a variational approach based upon Gutzwiller-projected fermionic Ans\"atze. Our results suggest that the Dirac spin liquid is stable for small spin-phonon couplings, while valence-bond solids are obtained at large couplings. Even though different distortions can be induced by the spin-phonon interaction, the general aspect is that the energy is lowered by maximizing the density of perfect hexagons in the dimerization pattern.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Topological Materials and Phenomena
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute for Theoretical Physics, Goethe University Frankfurt, Max-von-Laue-Straße 1, D-60438 Frankfurt a.M., Germany
Dipartimento di Fisica, Università di Trieste, Strada Costiera 11, I-34151 Trieste, Italy
Funding
Deutsche Forschungsgemeinschaft
References (56)
Show source-provided references
1. G. Misguich · 200510.1142/9789812567819_0005 ↗
2. 10.1103/PhysRevB.46.1420110.1103/PhysRevB.46.14201 ↗
3. 10.1103/PhysRevLett.68.176610.1103/PhysRevLett.68.1766 ↗
4. 10.1103/PhysRevB.47.545910.1103/PhysRevB.47.5459 ↗
5. 10.1103/PhysRevB.45.1237710.1103/PhysRevB.45.12377 ↗
6. 10.1063/1.34783010.1063/1.347830 ↗
7. 10.1103/PhysRevB.68.21441510.1103/PhysRevB.68.214415 ↗
8. 10.1103/PhysRevB.76.18040710.1103/PhysRevB.76.180407 ↗
9. 10.1103/PhysRevB.84.21440110.1103/PhysRevB.84.214401 ↗
10. 10.1103/PhysRevB.77.14441510.1103/PhysRevB.77.144415 ↗
11. 10.1103/PhysRevB.81.18040210.1103/PhysRevB.81.180402 ↗
12. 10.1103/PhysRevB.56.252110.1103/PhysRevB.56.2521 ↗
13. 10.1103/PhysRevLett.81.235610.1103/PhysRevLett.81.2356 ↗
14. 10.1007/PL0001107110.1007/PL00011071 ↗
15. 10.1103/PhysRevB.100.15514210.1103/PhysRevB.100.155142 ↗
16. 10.1103/PhysRevB.51.831810.1103/PhysRevB.51.8318 ↗
17. 10.1103/PhysRevLett.101.11720310.1103/PhysRevLett.101.117203 ↗
18. 10.1126/science.120108010.1126/science.1201080 ↗
19. 10.1103/PhysRevLett.109.06720110.1103/PhysRevLett.109.067201 ↗
20. 10.1103/PhysRevB.87.06040510.1103/PhysRevB.87.060405 ↗
21. 10.1103/PhysRevLett.98.11720510.1103/PhysRevLett.98.117205 ↗
22. 10.1103/PhysRevB.65.16511310.1103/PhysRevB.65.165113 ↗
23. 10.1088/1367-2630/14/11/11503110.1088/1367-2630/14/11/115031 ↗
24. 10.1103/PhysRevB.84.02040710.1103/PhysRevB.84.020407 ↗
25. 10.1103/PhysRevX.7.03102010.1103/PhysRevX.7.031020 ↗
26. 10.1126/sciadv.aat553510.1126/sciadv.aat5535 ↗
27. 10.1103/PhysRevB.103.19514010.1103/PhysRevB.103.195140 ↗
28. 10.1103/PhysRevLett.118.13720210.1103/PhysRevLett.118.137202 ↗
29. 10.1038/s41467-019-11727-310.1038/s41467-019-11727-3 ↗
30. 10.1103/PhysRevB.63.01441310.1103/PhysRevB.63.014413 ↗
31. 10.1103/PhysRevB.77.22441310.1103/PhysRevB.77.224413 ↗
32. 10.1103/PhysRevX.10.01103310.1103/PhysRevX.10.011033 ↗
33. 10.1103/PhysRevB.91.07511210.1103/PhysRevB.91.075112 ↗
34. 10.1103/PhysRevB.91.10441810.1103/PhysRevB.91.104418 ↗
35. 10.1103/PhysRevB.104.14440610.1103/PhysRevB.104.144406 ↗
36. 10.1103/PhysRevB.102.02041110.1103/PhysRevB.102.020411 ↗
37. 10.1103/PhysRevResearch.5.L01202510.1103/PhysRevResearch.5.L012025 ↗
38. 10.1103/PhysRevB.19.40210.1103/PhysRevB.19.402 ↗
39. 10.1103/PhysRevB.10.463710.1103/PhysRevB.10.4637 ↗
40. 10.1103/PhysRevB.57.R1400410.1103/PhysRevB.57.R14004 ↗
41. 10.1103/PhysRevLett.83.40810.1103/PhysRevLett.83.408 ↗
42. 10.1103/PhysRevLett.83.19510.1103/PhysRevLett.83.195 ↗
43. 10.1103/PhysRevB.102.12514910.1103/PhysRevB.102.125149 ↗
44. 10.1103/PhysRevResearch.2.03318010.1103/PhysRevResearch.2.033180 ↗
45. 10.1103/PhysRevB.105.16515110.1103/PhysRevB.105.165151 ↗
46. 10.1103/PhysRevB.107.21442810.1103/PhysRevB.107.214428 ↗
47. 10.1103/PhysRevB.104.03512610.1103/PhysRevB.104.035126 ↗
48. 10.1103/PhysRevLett.93.10720610.1103/PhysRevLett.93.107206 ↗
49. 10.1103/PhysRevLett.42.169810.1103/PhysRevLett.42.1698 ↗
50. 10.1103/PhysRevB.106.L08110710.1103/PhysRevB.106.L081107 ↗
51. 10.1103/PhysicsPhysiqueFizika.2.510.1103/PhysicsPhysiqueFizika.2.5 ↗
52. 10.1088/0034-4885/80/1/01650210.1088/0034-4885/80/1/016502 ↗
53. 10.1103/PhysRevB.71.24110310.1103/PhysRevB.71.241103 ↗
54. 10.1103/PhysRevB.83.22441310.1103/PhysRevB.83.224413 ↗
55. 10.1103/PhysRevLett.104.18720310.1103/PhysRevLett.104.187203 ↗
56. 10.1103/PhysRevB.84.09441910.1103/PhysRevB.84.094419 ↗