Emergence of Kac-Moody symmetry in critical quantum spin chains
Source abstract
Abstract
Given a critical quantum spin chain with a microscopic Lie group symmetry, corresponding, e.g., to $U(1)$ or $SU(2)$ spin isotropy, we numerically investigate the emergence of Kac-Moody symmetry at low energies and long distances. In that regime, one such critical quantum spin chain is described by a conformal field theory where the usual Virasoro algebra associated with conformal invariance is augmented with a Kac-Moody algebra associated with conserved currents. Specifically, we first propose a method to construct lattice operators corresponding to the Kac-Moody generators. We then numerically show that, when projected onto low-energy states of the quantum spin chain, these operators indeed approximately fulfill the Kac-Moody algebra. The lattice version of the Kac-Moody generators allows us to compute the so-called level constant and to organize the low-energy eigenstates of the lattice Hamiltonian into Kac-Moody towers. We illustrate the proposal with the XXZ model and the Heisenberg model with a next-to-nearest-neighbor coupling.
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Research context
OpenAlex topics: Algebraic structures and combinatorial models · Physics of Superconductivity and Magnetism · Quantum many-body systems
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References (30)
Show source-provided references
1. 10.1016/0370-1573(74)90023-410.1016/0370-1573(74)90023-4 ↗
2. 10.1103/PhysRevLett.52.157510.1103/PhysRevLett.52.1575 ↗
3. 10.1016/0550-3213(84)90052-X10.1016/0550-3213(84)90052-X ↗
4. 10.1088/0305-4470/17/7/00310.1088/0305-4470/17/7/003 ↗
5. 10.1103/PhysRevLett.56.74210.1103/PhysRevLett.56.742 ↗
6. 10.1103/PhysRevLett.56.74610.1103/PhysRevLett.56.746 ↗
7. 10.1016/0550-3213(86)90552-310.1016/0550-3213(86)90552-3 ↗
8. 10.1016/0550-3213(94)90018-310.1016/0550-3213(94)90018-3 ↗
9. 10.1016/j.nuclphysb.2007.03.03310.1016/j.nuclphysb.2007.03.033 ↗
10. 10.1016/j.nuclphysb.2010.02.01610.1016/j.nuclphysb.2010.02.016 ↗
11. 10.1088/1751-8113/46/49/49401210.1088/1751-8113/46/49/494012 ↗
12. 10.1016/j.nuclphysb.2012.11.00410.1016/j.nuclphysb.2012.11.004 ↗
13. 10.1088/1751-8113/48/6/06520510.1088/1751-8113/48/6/065205 ↗
14. 10.1103/PhysRevB.96.24510510.1103/PhysRevB.96.245105 ↗
15. 10.1103/PhysRevLett.121.23040210.1103/PhysRevLett.121.230402 ↗
16. 10.1103/PhysRevLett.124.04060410.1103/PhysRevLett.124.040604 ↗
17. 10.1103/PhysRevLett.115.16640110.1103/PhysRevLett.115.166401 ↗
18. 10.1103/PhysRevLett.120.20640310.1103/PhysRevLett.120.206403 ↗
19. 10.1016/0550-3213(87)90166-010.1016/0550-3213(87)90166-0 ↗
20. 10.1023/A:100489470190010.1023/A:1004894701900 ↗
21. 10.1103/PhysRevB.25.218510.1103/PhysRevB.25.2185 ↗
22. 10.1103/PhysRevB.41.1283810.1103/PhysRevB.41.12838 ↗
23. 10.1007/BF0123885710.1007/BF01238857 ↗
24. P. Francesco · 2012
25. R. Blumenhagen · 200910.1007/978-3-642-00450-6 ↗
26. 10.1103/PhysRevB.101.04513210.1103/PhysRevB.101.045132 ↗
27. E. Fradkin · 201310.1017/CBO9781139015509 ↗
28. 10.1006/aphy.1995.110110.1006/aphy.1995.1101 ↗
29. 10.1088/0305-4470/22/5/01510.1088/0305-4470/22/5/015 ↗
30. 10.1103/PhysRevB.54.R961210.1103/PhysRevB.54.R9612 ↗