STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface
Autor(a) principal: | |
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Data de Publicação: | 2004 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Brazilian Journal of Physics |
Texto Completo: | http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000400025 |
Resumo: | Bi-covered (<FONT FACE=Symbol>Ö</font>3× <FONT FACE=Symbol>Ö</font>3) reconstructed Si(111) surface has been studied by first principles calculations. Three different Bi coverages have been considered: 1 monolayer (ML), 1/3 ML and 2/3 ML, leading to the milkstool, T4 and the honeycomb structural models, respectively. Our total energy calculations show that the milkstool model is the energetically most stable structure for high Bi coverages followed by the T4 model for low Bi coverages, without going through a stable structure for the honeycomb model. We performed theoretical STM simulations for the three structures. For 1 ML coverage we observe the formation of Bi-trimers for occupied states, and a honeycomb image for empty states. It is suggested that the experimentally obtained STM image of a honeycomb structure does not correspond to a Bi-coverage of 2/3 ML, but it could represent a STM image of empty states localized in the T4 sites aside the Bi-trimers of the milkstool model. |
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Brazilian Journal of Physics |
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spelling |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surfaceBi-covered (<FONT FACE=Symbol>Ö</font>3× <FONT FACE=Symbol>Ö</font>3) reconstructed Si(111) surface has been studied by first principles calculations. Three different Bi coverages have been considered: 1 monolayer (ML), 1/3 ML and 2/3 ML, leading to the milkstool, T4 and the honeycomb structural models, respectively. Our total energy calculations show that the milkstool model is the energetically most stable structure for high Bi coverages followed by the T4 model for low Bi coverages, without going through a stable structure for the honeycomb model. We performed theoretical STM simulations for the three structures. For 1 ML coverage we observe the formation of Bi-trimers for occupied states, and a honeycomb image for empty states. It is suggested that the experimentally obtained STM image of a honeycomb structure does not correspond to a Bi-coverage of 2/3 ML, but it could represent a STM image of empty states localized in the T4 sites aside the Bi-trimers of the milkstool model.Sociedade Brasileira de Física2004-06-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000400025Brazilian Journal of Physics v.34 n.2b 2004reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332004000400025info:eu-repo/semantics/openAccessSchmidt,T. M.Miwa,R. H.Srivastava,G. P.eng2004-08-31T00:00:00Zoai:scielo:S0103-97332004000400025Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2004-08-31T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false |
dc.title.none.fl_str_mv |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
title |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
spellingShingle |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface Schmidt,T. M. |
title_short |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
title_full |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
title_fullStr |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
title_full_unstemmed |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
title_sort |
STM images and energetics of the bi-covered (Ö3 × Ö3) reconstructed Si(111) surface |
author |
Schmidt,T. M. |
author_facet |
Schmidt,T. M. Miwa,R. H. Srivastava,G. P. |
author_role |
author |
author2 |
Miwa,R. H. Srivastava,G. P. |
author2_role |
author author |
dc.contributor.author.fl_str_mv |
Schmidt,T. M. Miwa,R. H. Srivastava,G. P. |
description |
Bi-covered (<FONT FACE=Symbol>Ö</font>3× <FONT FACE=Symbol>Ö</font>3) reconstructed Si(111) surface has been studied by first principles calculations. Three different Bi coverages have been considered: 1 monolayer (ML), 1/3 ML and 2/3 ML, leading to the milkstool, T4 and the honeycomb structural models, respectively. Our total energy calculations show that the milkstool model is the energetically most stable structure for high Bi coverages followed by the T4 model for low Bi coverages, without going through a stable structure for the honeycomb model. We performed theoretical STM simulations for the three structures. For 1 ML coverage we observe the formation of Bi-trimers for occupied states, and a honeycomb image for empty states. It is suggested that the experimentally obtained STM image of a honeycomb structure does not correspond to a Bi-coverage of 2/3 ML, but it could represent a STM image of empty states localized in the T4 sites aside the Bi-trimers of the milkstool model. |
publishDate |
2004 |
dc.date.none.fl_str_mv |
2004-06-01 |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000400025 |
url |
http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332004000400025 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
10.1590/S0103-97332004000400025 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
text/html |
dc.publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
publisher.none.fl_str_mv |
Sociedade Brasileira de Física |
dc.source.none.fl_str_mv |
Brazilian Journal of Physics v.34 n.2b 2004 reponame:Brazilian Journal of Physics instname:Sociedade Brasileira de Física (SBF) instacron:SBF |
instname_str |
Sociedade Brasileira de Física (SBF) |
instacron_str |
SBF |
institution |
SBF |
reponame_str |
Brazilian Journal of Physics |
collection |
Brazilian Journal of Physics |
repository.name.fl_str_mv |
Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF) |
repository.mail.fl_str_mv |
sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br |
_version_ |
1754734861053067264 |