Bias-Free Access to Orbital Angular Momentum in Two-Dimensional Quantum Materials

The demonstration of a topological band inversion constitutes the most elementary proof of a quantum spin Hall insulator (QSHI). On a fundamental level, such an inverted band gap is intrinsically related to the bulk Berry curvature, a gauge-invariant fingerprint of the wave function's quantum g...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Physical review letters 2024-05, Vol.132 (19), p.196401-196401, Article 196401
Hauptverfasser: Erhardt, Jonas, Schmitt, Cedric, Eck, Philipp, Schmitt, Matthias, Keßler, Philipp, Lee, Kyungchan, Kim, Timur, Cacho, Cephise, Cojocariu, Iulia, Baranowski, Daniel, Feyer, Vitaliy, Veyrat, Louis, Sangiovanni, Giorgio, Claessen, Ralph, Moser, Simon
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:The demonstration of a topological band inversion constitutes the most elementary proof of a quantum spin Hall insulator (QSHI). On a fundamental level, such an inverted band gap is intrinsically related to the bulk Berry curvature, a gauge-invariant fingerprint of the wave function's quantum geometric properties in Hilbert space. Intimately tied to orbital angular momentum (OAM), the Berry curvature can be, in principle, extracted from circular dichroism in angle-resolved photoemission spectroscopy (CD-ARPES), were it not for interfering final state photoelectron emission channels that obscure the initial state OAM signature. Here, we outline a full-experimental strategy to avoid such interference artifacts and isolate the clean OAM from the CD-ARPES response. Bench-marking this strategy for the recently discovered atomic monolayer system indenene, we demonstrate its distinct QSHI character and establish CD-ARPES as a scalable bulk probe to experimentally classify the topology of two-dimensional quantum materials with time reversal symmetry.
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.132.196401