journal article·2021-01-29Open access

Bifurcating subsystem symmetric entanglement renormalization in two dimensions

Jonathan Francisco San Miguel, Arpit Dua, Dominic J. Williamson

Physical Review B· Volume 103· Issue 3

Abstract

We introduce the subsystem symmetry-preserving real-space entanglement renormalization group and apply it to study bifurcating flows generated by linear and fractal subsystem symmetry-protected topological phases in two spatial dimensions. We classify all bifurcating fixed points that are given by subsystem symmetric cluster states with two qubits per unit cell. In particular, we find that the square lattice cluster state is a quotient-bifurcating fixed point, while the cluster states derived from Yoshida's first-order fractal spin liquid models are self-bifurcating fixed points. We discuss the relevance of bifurcating subsystem symmetry-preserving renormalization group fixed points for the classification and equivalence of subsystem symmetry-protected topological phases.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum many-body systems · Quantum and electron transport phenomena · Physics of Superconductivity and Magnetism

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Physics, Stanford University, Stanford, California 94305, USA

Department of Physics, Yale University, New Haven, Connecticut 06520-8120, USA

Department of Physics and Institute for Quantum Information and Matter, California Institute of Technology, Pasadena, California 91125, USA

Funding

National Science Foundation

References (60)

Show source-provided references
1. 10.1142/S021797929000013910.1142/S0217979290000139 ↗
2. 10.1016/S0003-4916(02)00018-010.1016/S0003-4916(02)00018-0 ↗
3. 10.1103/RevModPhys.80.108310.1103/RevModPhys.80.1083 ↗
4. 10.1103/PhysRevB.87.15511410.1103/PhysRevB.87.155114 ↗
5. 10.1103/PhysRevLett.108.24050510.1103/PhysRevLett.108.240505 ↗
6. 10.1088/1367-2630/14/11/11301610.1088/1367-2630/14/11/113016 ↗
7. 10.1103/PhysRevLett.119.01050410.1103/PhysRevLett.119.010504 ↗
8. 10.1103/PhysRevA.96.01230210.1103/PhysRevA.96.012302 ↗
9. 10.1103/PhysRevLett.94.04040210.1103/PhysRevLett.94.040402 ↗
10. 10.1016/j.aop.2010.11.00210.1016/j.aop.2010.11.002 ↗
11. 10.1103/PhysRevA.83.04233010.1103/PhysRevA.83.042330 ↗
12. 10.1103/PhysRevLett.111.20050110.1103/PhysRevLett.111.200501 ↗
13. 10.1103/PhysRevB.94.23515710.1103/PhysRevB.94.235157 ↗
14. 10.1103/PhysRevResearch.2.01330310.1103/PhysRevResearch.2.013303 ↗
15. 10.1146/annurev-conmatphys-031218-01360410.1146/annurev-conmatphys-031218-013604 ↗
16. 10.1142/S0217751X2030003310.1142/S0217751X20300033 ↗
17. 10.1103/PhysRevLett.86.518810.1103/PhysRevLett.86.5188 ↗
18. 10.1038/nphys115710.1038/nphys1157 ↗
19. 10.1103/PhysRevLett.122.09050110.1103/PhysRevLett.122.090501 ↗
20. 10.1103/PhysRevB.98.03511210.1103/PhysRevB.98.035112 ↗
21. 10.21468/SciPostPhys.6.1.00710.21468/SciPostPhys.6.1.007 ↗
22. 10.1103/PhysRevA.98.02233210.1103/PhysRevA.98.022332 ↗
23. 10.22331/q-2019-05-20-14210.22331/q-2019-05-20-142 ↗
24. 10.1103/PhysRevLett.122.14050610.1103/PhysRevLett.122.140506 ↗
25. 10.22331/q-2020-02-10-22810.22331/q-2020-02-10-228 ↗
26. 10.1103/PhysRevLett.99.22040510.1103/PhysRevLett.99.220405 ↗
27. 10.1103/PhysRevB.89.07511910.1103/PhysRevB.89.075119 ↗
28. 10.1103/PhysRevX.8.03105110.1103/PhysRevX.8.031051 ↗
29. 10.1103/PhysRevResearch.2.03302110.1103/PhysRevResearch.2.033021 ↗
30. 10.1103/PhysRevB.83.03510710.1103/PhysRevB.83.035107 ↗
31. 10.1103/PhysRevB.84.16513910.1103/PhysRevB.84.165139 ↗
32. 10.1103/PhysRevB.80.15513110.1103/PhysRevB.80.155131 ↗
33. 10.1103/PhysRevResearch.2.04316510.1103/PhysRevResearch.2.043165 ↗
34. 10.21468/SciPostPhys.10.1.01110.21468/SciPostPhys.10.1.011 ↗
35. 10.1103/PhysRevB.98.23512110.1103/PhysRevB.98.235121 ↗
36. 10.1103/PhysRevB.99.23513110.1103/PhysRevB.99.235131 ↗
37. 10.1103/PhysRevB.102.11510310.1103/PhysRevB.102.115103 ↗
38. 10.1103/PhysRevResearch.2.01205910.1103/PhysRevResearch.2.012059 ↗
39. 10.1103/PhysRevB.88.12512210.1103/PhysRevB.88.125122 ↗
40. 10.1103/PhysRevB.88.12110810.1103/PhysRevB.88.121108 ↗
41. 10.1103/PhysRevB.88.20512410.1103/PhysRevB.88.205124 ↗
42. 10.1103/PhysRevLett.86.91010.1103/PhysRevLett.86.910 ↗
43. 10.1103/PhysRevA.68.02231210.1103/PhysRevA.68.022312 ↗
44. 10.1142/9789812798763_001110.1142/9789812798763_0011 ↗
45. 10.1103/RevModPhys.47.77310.1103/RevModPhys.47.773 ↗
46. 10.1088/0264-9381/30/11/11501510.1088/0264-9381/30/11/115015 ↗
47. 10.1103/PhysRevB.78.20511610.1103/PhysRevB.78.205116 ↗
48. 10.1103/PhysRevLett.100.07040410.1103/PhysRevLett.100.070404 ↗
49. 10.1103/PhysRevB.79.19512310.1103/PhysRevB.79.195123 ↗
50. 10.1103/PhysRevB.82.15513810.1103/PhysRevB.82.155138 ↗
51. 10.1103/PhysRevLett.112.22050210.1103/PhysRevLett.112.220502 ↗
52. 10.1103/PhysRevLett.112.24050210.1103/PhysRevLett.112.240502 ↗
53. 10.1103/PhysRevB.89.23511310.1103/PhysRevB.89.235113 ↗
54. 10.1103/PhysRevB.79.14410810.1103/PhysRevB.79.144108 ↗
55. 10.1070/1063-7869/44/10S/S2910.1070/1063-7869/44/10S/S29 ↗
56. 10.1103/PhysRevB.71.04511010.1103/PhysRevB.71.045110 ↗
57. 10.1103/PhysRevB.100.11514710.1103/PhysRevB.100.115147 ↗
58. 10.1103/PhysRevB.94.15512810.1103/PhysRevB.94.155128 ↗
59. 10.1103/PhysRevResearch.2.03333110.1103/PhysRevResearch.2.033331 ↗
60. 10.1007/s00220-013-1810-210.1007/s00220-013-1810-2 ↗