Exhaustive Characterization of Quantum Many-Body Scars Using Commutant Algebras
Abstract
We study quantum many-body scars (QMBS) in the language of commutant algebras, which are defined as symmetry algebras of families of local Hamiltonians. This framework explains the origin of dynamically disconnected subspaces seen in models with exact QMBS, i.e., the large “thermal” subspace and the small “nonthermal” subspace, which are attributed to the existence of unconventional nonlocal conserved quantities in the commutant; hence, it unifies the study of conventional symmetries and weak ergodicity-breaking phenomena into a single framework. Furthermore, this language enables us to use the von Neumann double commutant theorem to formally write down the exhaustive algebra of all Hamiltonians with a desired set of QMBS, which demonstrates that QMBS survive under large classes of local perturbations. We illustrate this using several standard examples of QMBS, including the spin-1/2 ferromagnetic, AKLT, spin-1 XY 𝜋-bimagnon, and the electronic 𝜂-pairing towers of states; in each of these cases, we explicitly write down a set of generators for the full algebra of Hamiltonians with these QMBS. Understanding this hidden structure in QMBS Hamiltonians also allows us to recover results of previous “brute-force” numerical searches for such Hamiltonians. In addition, this language clearly demonstrates the equivalence of several unified formalisms for QMBS proposed in the literature and also illustrates the connection between two apparently distinct classes of QMBS Hamiltonians—those that are captured by the so-called Shiraishi-Mori construction and those that lie beyond. Finally, we show that this framework motivates a precise definition for QMBS that automatically implies that they violate the conventional eigenstate thermalization hypothesis, and we discuss its implications to dynamics.
Copyright and License
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
Acknowledgement
We thank David Huse, Hosho Katsura, Igor Klebanov, Nick O’Dea, Kiryl Pakrouski, and Marcos Rigol for useful discussions. S. M. particularly thanks Nicolas Regnault and B. Andrei Bernevig for previous collaborations on related topics, while O. I. M. thanks Daniel Mark and Cheng-Ju Lin. This work was supported by the Walter Burke Institute for Theoretical Physics at Caltech; the Institute for Quantum Information and Matter, a National Science Foundation Physics Frontiers Center (Grant No. PHY-1733907); the National Science Foundation through Grant No. DMR-2001186; and Munich Center for Quantum Science and Technology (MCQST). Part of this work was carried out at the Aspen Center for Physics, which is supported by National Science Foundation Grant No. PHY-1607611. This work was partially supported by a grant from the Simons Foundation.
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Additional details
- California Institute of Technology
- National Science Foundation
- PHY-1733907
- National Science Foundation
- DMR-2001186
- Munich Center for Quantum Science and Technology
- National Science Foundation
- PHY-1607611
- Simons Foundation
- Accepted
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2024-10-30Accepted
- Caltech groups
- Institute for Quantum Information and Matter, Walter Burke Institute for Theoretical Physics
- Publication Status
- Published