Rydberg series of dark excitons and the conduction band spin-orbit splitting in monolayer WSe2
dc.contributor.author | Kapuscinski, Piotr | cs |
dc.contributor.author | Delhomme, Alex | cs |
dc.contributor.author | Václavková, Diana | cs |
dc.contributor.author | Slobodeniuk, Artur | cs |
dc.contributor.author | Grzeszczyk, Magdalena | cs |
dc.contributor.author | Bartoš, Miroslav | cs |
dc.contributor.author | Watanabe, Kenji | cs |
dc.contributor.author | Taniguchi, Takashi | cs |
dc.contributor.author | Faugeras, Clément | cs |
dc.contributor.author | Potemski, Marek | cs |
dc.coverage.issue | 1 | cs |
dc.coverage.volume | 4 | cs |
dc.date.issued | 2021-08-19 | cs |
dc.description.abstract | Strong Coulomb correlations together with multi-valley electronic bands in the presence of spin-orbit interaction are at the heart of studies of the rich physics of excitons in monolayers of transition metal dichalcogenides (TMD). Those archetypes of two-dimensional systems promise a design of new optoelectronic devices. In intrinsic TMD monolayers the basic, intravalley excitons, are formed by a hole from the top of the valence band and an electron either from the lower or upper spin-orbit-split conduction band subbands: one of these excitons is optically active, the second one is dark, although possibly observed under special conditions. Here we demonstrate the s-series of Rydberg dark exciton states in tungsten diselenide monolayer, which appears in addition to a conventional bright exciton series in photoluminescence spectra measured in high in-plane magnetic fields. The comparison of energy ladders of bright and dark Rydberg excitons is shown to be a method to experimentally evaluate one of the missing band parameters in TMD monolayers: the amplitude of the spin-orbit splitting of the conduction band. Excitonic physics dominates the optical response of semiconductor monolayers but single particle band structure parameters are hard to probe experimentally. Here, spin-orbit splitting in the conduction band of monolayer WSe2 is revealed by the identification of the Rydberg series of dark excitons. | en |
dc.format | text | cs |
dc.format.extent | 186-1-186-6 | cs |
dc.format.mimetype | application/pdf | cs |
dc.identifier.citation | COMMUNICATIONS PHYSICS. 2021, vol. 4, issue 1, p. 186-1-186-6. | en |
dc.identifier.doi | 10.1038/s42005-021-00692-3 | cs |
dc.identifier.issn | 2399-3650 | cs |
dc.identifier.orcid | 0000-0002-5923-0260 | cs |
dc.identifier.other | 173163 | cs |
dc.identifier.researcherid | B-3350-2014 | cs |
dc.identifier.uri | http://hdl.handle.net/11012/203058 | |
dc.language.iso | en | cs |
dc.publisher | NATURE PORTFOLIO | cs |
dc.relation.ispartof | COMMUNICATIONS PHYSICS | cs |
dc.relation.uri | https://www.nature.com/articles/s42005-021-00692-3 | cs |
dc.rights | Creative Commons Attribution 4.0 International | cs |
dc.rights.access | openAccess | cs |
dc.rights.sherpa | http://www.sherpa.ac.uk/romeo/issn/2399-3650/ | cs |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | cs |
dc.subject | PHOTOLUMINESCENCE | en |
dc.title | Rydberg series of dark excitons and the conduction band spin-orbit splitting in monolayer WSe2 | en |
dc.type.driver | article | en |
dc.type.status | Peer-reviewed | en |
dc.type.version | publishedVersion | en |
sync.item.dbid | VAV-173163 | en |
sync.item.dbtype | VAV | en |
sync.item.insts | 2025.02.03 15:50:49 | en |
sync.item.modts | 2025.01.17 19:35:35 | en |
thesis.grantor | Vysoké učení technické v Brně. Středoevropský technologický institut VUT. Magneto-Optická a THz Spektroskopie | cs |
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