Open momentum space method for the Hofstadter butterfly and the quantized Lorentz susceptibility
Source abstract
Abstract
We develop a generic $\mathbf{k}\ifmmode\cdot\else\textperiodcentered\fi{}\mathbf{p}$ open momentum space method for calculating the Hofstadter butterfly of both continuum (moir\'e) models and tight-binding models, where the quasimomentum is directly substituted by the Landau level (LL) operators. By taking a LL cutoff (and a reciprocal lattice cutoff for continuum models), one obtains the Hofstadter butterfly with in-gap spectral flows. For continuum models such as the moir\'e model for twisted bilayer graphene, our method gives a sparse Hamiltonian, making it much more efficient than existing methods. The spectral flows in the Hofstadter gaps can be understood as edge states on a momentum space boundary, from which one can determine the two integers (${t}_{\ensuremath{\nu}},{s}_{\ensuremath{\nu}}$) of a gap $\ensuremath{\nu}$ satisfying the Diophantine equation. The spectral flows can also be removed to obtain a clear Hofstadter butterfly. While ${t}_{\ensuremath{\nu}}$ is known as the Chern number, our theory identifies ${s}_{\ensuremath{\nu}}$ as a dual Chern number for the momentum space, which corresponds to a quantized Lorentz susceptibility ${\ensuremath{\gamma}}xy=eB{s}_{\ensuremath{\nu}}$.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Noncommutative and Quantum Gravity Theories · Algebraic structures and combinatorial models
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics, Princeton University, Princeton, New Jersey 08544, USA
Funding
U.S. Department of Energy · National Science Foundation · Office of Naval Research · Gordon and Betty Moore Foundation
References (28)
Show source-provided references
1. 10.1103/PhysRevB.14.223910.1103/PhysRevB.14.2239 ↗
2. 10.1073/pnas.110817410810.1073/pnas.1108174108 ↗
3. 10.1103/PhysRevLett.99.25680210.1103/PhysRevLett.99.256802 ↗
4. 10.1103/PhysRevB.81.16140510.1103/PhysRevB.81.161405 ↗
5. 10.1103/PhysRevB.84.03544010.1103/PhysRevB.84.035440 ↗
6. 10.1103/PhysRevB.87.23542910.1103/PhysRevB.87.235429 ↗
7. 10.1103/PhysRevB.89.24140710.1103/PhysRevB.89.241407 ↗
8. 10.1103/PhysRevB.100.03511510.1103/PhysRevB.100.035115 ↗
9. 10.1103/PhysRevB.100.12510410.1103/PhysRevB.100.125104 ↗
10. 10.1103/PhysRevLett.49.40510.1103/PhysRevLett.49.405 ↗
11. R. Winkler · 200310.1007/b13586 ↗
12. 10.1103/PhysRevB.102.04140210.1103/PhysRevB.102.041402 ↗
13. 10.1103/PhysRevLett.118.21680110.1103/PhysRevLett.118.216801 ↗
14. 10.1103/PhysRevB.19.606810.1103/PhysRevB.19.6068 ↗
15. 10.1088/0022-3719/18/22/00410.1088/0022-3719/18/22/004 ↗
16. I. I. Satija · 201610.1088/978-1-6817-4117-8 ↗
17. 10.1103/PhysRevResearch.1.03307610.1103/PhysRevResearch.1.033076 ↗
18. 10.1002/pssb.222088024310.1002/pssb.2220880243 ↗
19. 10.1088/0022-3719/15/22/00510.1088/0022-3719/15/22/005 ↗
20. 10.1103/PhysRev.84.81410.1103/PhysRev.84.814 ↗
21. 10.1143/JPSJ.74.281310.1143/JPSJ.74.2813 ↗
22. 10.1103/PhysRevB.97.14442210.1103/PhysRevB.97.144422 ↗
23. 10.1103/PhysRevLett.125.23680410.1103/PhysRevLett.125.236804 ↗
24. 10.1126/science.aaw378010.1126/science.aaw3780 ↗
25. 10.1126/science.aay553310.1126/science.aay5533 ↗
26. 10.1103/PhysRevLett.123.03640110.1103/PhysRevLett.123.036401 ↗
27. B. A. Bernevig · 201310.1515/9781400846733 ↗
28. 10.1103/PhysRev.95.115410.1103/PhysRev.95.1154 ↗