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dc.contributor.authorPeelaers, Hartwin
dc.contributor.authorKioupakis, E.
dc.contributor.authorVan de Walle, C. G.
dc.date.accessioned2021-04-12T20:19:03Z
dc.date.available2021-04-12T20:19:03Z
dc.date.issued2019-08-23
dc.identifier.citationH. Peelaers, E. Kioupakis, and C. G. Van de Walle , "Limitations of In2O3 as a transparent conducting oxide", Applied Physics Letters 115, 082105 (2019) https://doi.org/10.1063/1.5109569en_US
dc.identifier.urihttp://hdl.handle.net/1808/31588
dc.descriptionThis article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in Appl. Phys. Lett. 115, 082105 (2019); doi: 10.1063/1.5109569 and may be found at https://aip.scitation.org/doi/full/10.1063/1.5109569.en_US
dc.description.abstractSn-doped In2O3 or ITO is the most widely used transparent conducting oxide. We use first-principles calculations to investigate the limitations to its transparency due to free-carrier absorption mediated by phonons or charged defects. We find that the main contribution to the phonon-assisted indirect absorption is due to emission (as opposed to absorption) of phonons, which explains why the process is relatively insensitive to temperature. The wavelength dependence of this indirect absorption process can be described by a power law. Indirect absorption mediated by charged defects or impurities is also unavoidable since doping is required to obtain conductivity. At high carrier concentrations, screening by the free carriers becomes important. We find that charged-impurity-assisted absorption becomes larger than phonon-assisted absorption for impurity concentrations above 1020 cm–3. The differences in the photon-energy dependence of the two processes can be explained by band structure effects.en_US
dc.publisherAmerican Institute of Physicsen_US
dc.rights© 2019 Author(s). Published under license by AIP Publishing.en_US
dc.titleLimitations of In2O3 as a transparent conducting oxideen_US
dc.typeArticleen_US
kusw.kuauthorPeelaers, Hartwin
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1063/1.5109569en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-7141-8688en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-1880-6443en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-4212-5990en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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