Unwinding fermionic symmetry-protected topological phases: Supersymmetry extension
Source abstract
Abstract
We show how $1+1$-dimensional fermionic symmetry-protected topological states (SPTs, i.e., nontrivial short-range entangled gapped phases of quantum matter whose boundary exhibits 't Hooft anomaly and whose bulk cannot be deformed into a trivial tensor product state under finite-depth local unitary transformations only in the presence of global symmetries), indeed can be unwound to a trivial state by enlarging the Hilbert space via adding extra degrees of freedom and suitably extending the global symmetries. The extended projective global symmetry on the boundary can become supersymmetric in a specific sense, i.e., it contains group elements that do not commute with the fermion number parity ${(\ensuremath{-}1)}F$, while the antiunitary time-reversal symmetry becomes fractionalized. This also means we can uplift and remove certain exotic fermionic anomalies (e.g., ``parity'' anomaly in time-reversal or reflection symmetry) via appropriate supersymmetry extensions in terms of group extensions. We work out explicit examples for multilayers of $1+1\mathrm{d}$ Majorana fermion chains, then comment on models with Sachdev-Ye-Kitaev (SYK) interactions, intrinsic fermionic gapless SPTs protected by supersymmetry, and generalizations to higher space-time dimensions via a cobordism theory.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Quantum many-body systems · Quantum and electron transport phenomena
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Shivakote, Hesaraghatta, Bangalore 560089, India
Center of Mathematical Sciences and Applications, Harvard University, Cambridge, Massachusetts 02138, USA
School of Natural Sciences, Institute for Advanced Study, Einstein Drive, Princeton, New Jersey 08540, USA
Funding
National Science Foundation
References (67)
Show source-provided references
1. 10.1103/PhysRevB.87.15511410.1103/PhysRevB.87.155114 ↗
2. 10.1146/annurev-conmatphys-031214-01474010.1146/annurev-conmatphys-031214-014740 ↗
3. 10.1103/PhysRevB.98.12510810.1103/PhysRevB.98.125108 ↗
4. 10.1103/PhysRevX.8.03104810.1103/PhysRevX.8.031048 ↗
5. 10.1103/PhysRevB.94.19515010.1103/PhysRevB.94.195150 ↗
6. 10.21468/SciPostPhys.8.1.01510.21468/SciPostPhys.8.1.015 ↗
7. 10.21468/SciPostPhys.6.1.00310.21468/SciPostPhys.6.1.003 ↗
8. 10.1103/PhysRevX.3.01101610.1103/PhysRevX.3.011016 ↗
9. 10.1103/PhysRevX.3.04101610.1103/PhysRevX.3.041016 ↗
10. 10.1103/PhysRevLett.59.79910.1103/PhysRevLett.59.799 ↗
11. 10.1016/0003-4916(61)90115-410.1016/0003-4916(61)90115-4 ↗
12. 10.1103/PhysRevLett.70.333910.1103/PhysRevLett.70.3339 ↗
13. 10.4310/AMSA.2019.v4.n2.a210.4310/AMSA.2019.v4.n2.a2 ↗
14. 10.1063/1.314948110.1063/1.3149481 ↗
15. 10.1063/1.314949510.1063/1.3149495 ↗
16. 10.1103/PhysRevB.90.11514110.1103/PhysRevB.90.115141 ↗
17. 10.1007/JHEP10(2017)08010.1007/JHEP10(2017)080 ↗
18. 10.1103/PhysRevX.8.01105510.1103/PhysRevX.8.011055 ↗
19. 10.1007/JHEP05(2019)00710.1007/JHEP05(2019)007 ↗
20. 10.1103/PhysRevX.10.03105510.1103/PhysRevX.10.031055 ↗
21. 10.1007/JHEP12(2015)05210.1007/JHEP12(2015)052 ↗
22. 10.1016/j.aop.2018.04.02510.1016/j.aop.2018.04.025 ↗
23. 10.1007/s00220-019-03671-610.1007/s00220-019-03671-6 ↗
24. 10.1103/RevModPhys.88.03500510.1103/RevModPhys.88.035005 ↗
25. 10.1103/PhysRevLett.114.03160110.1103/PhysRevLett.114.031601 ↗
26. 10.1103/RevModPhys.89.04100410.1103/RevModPhys.89.041004 ↗
27. 10.1070/1063-7869/44/10S/S2910.1070/1063-7869/44/10S/S29 ↗
28. 10.1103/PhysRevB.81.13450910.1103/PhysRevB.81.134509 ↗
29. 10.1103/PhysRevB.83.07510310.1103/PhysRevB.83.075103 ↗
30. 10.1103/PhysRevResearch.2.03329010.1103/PhysRevResearch.2.033290 ↗
31. 10.1103/PhysRevB.98.16510410.1103/PhysRevB.98.165104 ↗
32. E. Witten · 1983
33. 10.1016/0370-1573(94)00080-M10.1016/0370-1573(94)00080-M ↗
34. 10.1016/0550-3213(81)90006-710.1016/0550-3213(81)90006-7 ↗
35. 10.1016/0550-3213(82)90071-210.1016/0550-3213(82)90071-2 ↗
36. 10.4310/jdg/121443749210.4310/jdg/1214437492 ↗
37. 10.1103/PhysRevLett.124.23680410.1103/PhysRevLett.124.236804 ↗
38. 10.1103/PhysRevB.98.12510110.1103/PhysRevB.98.125101 ↗
39. 10.1103/PhysRevB.95.11515010.1103/PhysRevB.95.115150 ↗
40. 10.1103/PhysRevD.94.10600210.1103/PhysRevD.94.106002 ↗
41. 10.1007/JHEP05(2018)18310.1007/JHEP05(2018)183 ↗
42. 10.4310/AMSA.2020.v5.n2.a210.4310/AMSA.2020.v5.n2.a2 ↗
43. 10.1103/PhysRevLett.124.12160110.1103/PhysRevLett.124.121601 ↗
44. 10.21468/SciPostPhys.9.1.01010.21468/SciPostPhys.9.1.010 ↗
45. 10.21468/SciPostPhys.7.5.05810.21468/SciPostPhys.7.5.058 ↗
46. 10.21468/SciPostPhys.8.4.06210.21468/SciPostPhys.8.4.062 ↗
47. 10.1142/S0217751X1830029610.1142/S0217751X18300296 ↗
48. 10.1016/j.aop.2017.06.01910.1016/j.aop.2017.06.019 ↗
49. 10.1007/JHEP08(2019)00310.1007/JHEP08(2019)003 ↗
50. 10.1007/JHEP07(2020)06210.1007/JHEP07(2020)062 ↗
51. 10.1088/0256-307X/30/11/11110110.1088/0256-307X/30/11/111101 ↗
52. 10.1103/PhysRevB.91.12514710.1103/PhysRevB.91.125147 ↗
53. 10.1093/ptep/ptz11510.1093/ptep/ptz115 ↗
54. 10.1103/PhysRevResearch.2.02335610.1103/PhysRevResearch.2.023356 ↗
55. R. C. Kirby · London Mathematical Society Lecture Note Series · 1990 · 2 · 177
56. 10.1088/1367-2630/16/1/01304410.1088/1367-2630/16/1/013044 ↗
57. 10.1126/science.124825310.1126/science.1248253 ↗
58. 10.1103/PhysRevB.94.20510610.1103/PhysRevB.94.205106 ↗
59. 10.1103/PhysRevB.100.07515310.1103/PhysRevB.100.075153 ↗
60. 10.1007/JHEP01(2021)06310.1007/JHEP01(2021)063 ↗
61. 10.1007/JHEP02(2015)17210.1007/JHEP02(2015)172 ↗
62. 10.1103/PhysRevD.99.06501310.1103/PhysRevD.99.065013 ↗
63. 10.1016/j.aop.2020.16807410.1016/j.aop.2020.168074 ↗
64. 10.1103/PhysRevD.100.08501210.1103/PhysRevD.100.085012 ↗
65. 10.1093/ptep/pty05110.1093/ptep/pty051 ↗
66. 10.1007/JHEP11(2019)13110.1007/JHEP11(2019)131 ↗
67. 10.21468/SciPostPhys.4.4.02110.21468/SciPostPhys.4.4.021 ↗