Please use this identifier to cite or link to this item: http://ricaxcan.uaz.edu.mx/jspui/handle/20.500.11845/617
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dc.contributor39945es_ES
dc.contributor.otherhttps://orcid.org/0000-0003-0087-8991-
dc.coverage.spatialGlobales_ES
dc.creatordel Río de Santiago, Antonio-
dc.creatorMartínez Orozco, Juan Carlos-
dc.creatorRodríguez Magdaleno, Karla Arely-
dc.creatorContreras Solorio, David Armando-
dc.creatorRodríguez Vargas, Isaac-
dc.creatorUngan, Fatih-
dc.date.accessioned2018-08-08T16:37:27Z-
dc.date.available2018-08-08T16:37:27Z-
dc.date.issued2018-03-
dc.identifierinfo:eu-repo/semantics/publishedVersiones_ES
dc.identifier.issn0749-6036es_ES
dc.identifier.urihttp://hdl.handle.net/20.500.11845/617-
dc.identifier.urihttps://doi.org/10.48779/q5s1-9276-
dc.description.abstractIt is reported a numerical computation of the local density of states for a d-doped like QW superlattices of AlxGa1 xAs, as a possible heterostructure that, being integrated into a solar cell device design, can provide an intermediate band of allowed states to assist the absorption of photons with lower energies than that of the energy gap of the solar-cell constituent materials. This work was performed using the nearest neighbors sp3s tightbinding model including spin. The confining potential caused by the ionized donor impurities in d-doped impurities seeding that was obtained analytically within the lines of the Thomas-Fermi approximation was reproduced here by the Al concentration x variation. This potential is considered as an external perturbation in the tight-binding methodology and it is included in the diagonal terms of the tight-binding Hamiltonian. Special attention is paid to the width of the intermediate band caused by the change in the considered aluminium concentration x, the inter-well distance between d-doped like QW wells and the number of them in the superlattice. In general we can conclude that this kind of superlattices can be suitable for intermediate band formation for possible intermediateband solar cell design.es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.relationhttps://www.sciencedirect.com/science/article/pii/S0749603618300533?via%3Dihub#!es_ES
dc.relation.ispartofhttps://reader.elsevier.com/reader/sd/B6A72483DD36EDEC5DF9C035BAABF8ED6AB97A93210E430B16D8E9E84A94F19957C7758537E8A415DC833225ACE329D5es_ES
dc.relation.urigeneralPublices_ES
dc.rightsAtribución-NoComercial-CompartirIgual 3.0 Estados Unidos de América*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.sourceSuperlattices and Microstructures, Volume 115, March 2018, Pages 191-196es_ES
dc.subject.classificationCIENCIAS FISICO MATEMATICAS Y CIENCIAS DE LA TIERRA [1]es_ES
dc.subject.otherd-doped superlatticees_ES
dc.subject.otherIntermediate-bandes_ES
dc.subject.otherSolar cellses_ES
dc.titleIntermediate band formation in a d-doped like QW superlattices of GaAs/AlxGa1 xAs for solar cell designes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
Appears in Collections:*Documentos Académicos*-- UA Física



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