Indium-zinc-oxide nanobelts with superlattice structure

Indium-zinc-oxide (IZO) nanobelts have been grown by a thermal evaporation-deposition method with ZnO and In-2O_3 powders as precursors. The nanobelts have a superlattice structure that is explained by the formation of In-O and In/Zn-O layers, which appears to favor the formation of nanorings. X-ray...

Descripción completa

Detalles Bibliográficos
Autores: Alemán, B., Fernández Sánchez, Paloma, Piqueras De Noriega, Francisco Javier
Tipo de recurso: artículo
Fecha de publicación:2009
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/44220
Acceso en línea:https://hdl.handle.net/20.500.14352/44220
Access Level:acceso abierto
Palabra clave:538.9
Zno
Nanowires
Nanospirals
Growth
Física de materiales
id ES_60e4a2d81abdca4a8f2d68fd5402e15c
oai_identifier_str oai:docta.ucm.es:20.500.14352/44220
network_acronym_str ES
network_name_str España
repository_id_str
spelling Indium-zinc-oxide nanobelts with superlattice structureAlemán, B.Fernández Sánchez, PalomaPiqueras De Noriega, Francisco Javier538.9ZnoNanowiresNanospiralsGrowthFísica de materialesIndium-zinc-oxide (IZO) nanobelts have been grown by a thermal evaporation-deposition method with ZnO and In-2O_3 powders as precursors. The nanobelts have a superlattice structure that is explained by the formation of In-O and In/Zn-O layers, which appears to favor the formation of nanorings. X-ray analytical methods indicate that the approximate composition of the compound is Zn_4In_2O_7. Cathodoluminescence of the nanobelts in scanning electron microscope shows a dominant emission at 2.37 eV, which is suggested to be a characteristic band of the IZO structure.Amer Inst PhysicsUniversidad Complutense de Madrid20092009-07-0620092009-07-06journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/44220reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/442202026-06-02T12:44:21Z
dc.title.none.fl_str_mv Indium-zinc-oxide nanobelts with superlattice structure
title Indium-zinc-oxide nanobelts with superlattice structure
spellingShingle Indium-zinc-oxide nanobelts with superlattice structure
Alemán, B.
538.9
Zno
Nanowires
Nanospirals
Growth
Física de materiales
title_short Indium-zinc-oxide nanobelts with superlattice structure
title_full Indium-zinc-oxide nanobelts with superlattice structure
title_fullStr Indium-zinc-oxide nanobelts with superlattice structure
title_full_unstemmed Indium-zinc-oxide nanobelts with superlattice structure
title_sort Indium-zinc-oxide nanobelts with superlattice structure
dc.creator.none.fl_str_mv Alemán, B.
Fernández Sánchez, Paloma
Piqueras De Noriega, Francisco Javier
author Alemán, B.
author_facet Alemán, B.
Fernández Sánchez, Paloma
Piqueras De Noriega, Francisco Javier
author_role author
author2 Fernández Sánchez, Paloma
Piqueras De Noriega, Francisco Javier
author2_role author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 538.9
Zno
Nanowires
Nanospirals
Growth
Física de materiales
topic 538.9
Zno
Nanowires
Nanospirals
Growth
Física de materiales
description Indium-zinc-oxide (IZO) nanobelts have been grown by a thermal evaporation-deposition method with ZnO and In-2O_3 powders as precursors. The nanobelts have a superlattice structure that is explained by the formation of In-O and In/Zn-O layers, which appears to favor the formation of nanorings. X-ray analytical methods indicate that the approximate composition of the compound is Zn_4In_2O_7. Cathodoluminescence of the nanobelts in scanning electron microscope shows a dominant emission at 2.37 eV, which is suggested to be a characteristic band of the IZO structure.
publishDate 2009
dc.date.none.fl_str_mv 2009
2009-07-06
2009
2009-07-06
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/44220
url https://hdl.handle.net/20.500.14352/44220
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Amer Inst Physics
publisher.none.fl_str_mv Amer Inst Physics
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869409341706076160
score 15,300719