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High-order replica bands in monolayer FeSe/SrTiO(3) revealed by polarization-dependent photoemission spectroscopy

The mechanism of the enhanced superconductivity in monolayer FeSe/SrTiO(3) has been enthusiastically studied and debated over the past decade. One specific observation has been taken to be of central importance: the replica bands in the photoemission spectrum. Although suggestive of electron-phonon...

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Detalles Bibliográficos
Autores principales: Liu, Chong, Day, Ryan P., Li, Fengmiao, Roemer, Ryan L., Zhdanovich, Sergey, Gorovikov, Sergey, Pedersen, Tor M., Jiang, Juan, Lee, Sangjae, Schneider, Michael, Wong, Doug, Dosanjh, Pinder, Walker, Frederick J., Ahn, Charles H., Levy, Giorgio, Damascelli, Andrea, Sawatzky, George A., Zou, Ke
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8319137/
https://www.ncbi.nlm.nih.gov/pubmed/34321473
http://dx.doi.org/10.1038/s41467-021-24783-5
Descripción
Sumario:The mechanism of the enhanced superconductivity in monolayer FeSe/SrTiO(3) has been enthusiastically studied and debated over the past decade. One specific observation has been taken to be of central importance: the replica bands in the photoemission spectrum. Although suggestive of electron-phonon interaction in the material, the essence of these spectroscopic features remains highly controversial. In this work, we conduct angle-resolved photoemission spectroscopy measurements on monolayer FeSe/SrTiO(3) using linearly polarized photons. This configuration enables unambiguous characterization of the valence electronic structure with a suppression of the spectral background. We consistently observe high-order replica bands derived from various Fe 3d bands, similar to those observed on bare SrTiO(3). The intensity of the replica bands is unexpectedly high and different between d(xy) and d(yz) bands. Our results provide new insights on the electronic structure of this high-temperature superconductor and the physical origin of the photoemission replica bands.