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Ir(6)In(32)S(21), a polar, metal-rich semiconducting subchalcogenide

Subchalcogenides are uncommon, and their chemical bonding results from an interplay between metal–metal and metal–chalcogenide interactions. Herein, we present Ir(6)In(32)S(21), a novel semiconducting subchalcogenide compound that crystallizes in a new structure type in the polar P31m space group, w...

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Detalles Bibliográficos
Autores principales: Khoury, Jason F., He, Jiangang, Pfluger, Jonathan E., Hadar, Ido, Balasubramanian, Mahalingam, Stoumpos, Constantinos C., Zu, Rui, Gopalan, Venkatraman, Wolverton, Chris, Kanatzidis, Mercouri G.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Royal Society of Chemistry 2019
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8146499/
https://www.ncbi.nlm.nih.gov/pubmed/34123065
http://dx.doi.org/10.1039/c9sc05609b
Descripción
Sumario:Subchalcogenides are uncommon, and their chemical bonding results from an interplay between metal–metal and metal–chalcogenide interactions. Herein, we present Ir(6)In(32)S(21), a novel semiconducting subchalcogenide compound that crystallizes in a new structure type in the polar P31m space group, with unit cell parameters a = 13.9378(12) Å, c = 8.2316(8) Å, α = β = 90°, γ = 120°. The compound has a large band gap of 1.48(2) eV, and photoemission and Kelvin probe measurements corroborate this semiconducting behavior with a valence band maximum (VBM) of −4.95(5) eV, conduction band minimum of −3.47(5) eV, and a photoresponse shift of the Fermi level by ∼0.2 eV in the presence of white light. X-ray absorption spectroscopy shows absorption edges for In and Ir do not indicate clear oxidation states, suggesting that the numerous coordination environments of Ir(6)In(32)S(21) make such assignments ambiguous. Electronic structure calculations confirm the semiconducting character with a nearly direct band gap, and electron localization function (ELF) analysis suggests that the origin of the gap is the result of electron transfer from the In atoms to the S 3p and Ir 5d orbitals. DFT calculations indicate that the average hole effective masses near the VBM (1.19m(e)) are substantially smaller than the average electron masses near the CBM (2.51m(e)), an unusual feature for most semiconductors. The crystal and electronic structure of Ir(6)In(32)S(21), along with spectroscopic data, suggest that it is neither a true intermetallic nor a classical semiconductor, but somewhere in between those two extremes.