The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†

Detalhes bibliográficos
Autor(a) principal: Guedes-Sobrinho, Diego
Data de Publicação: 2022
Outros Autores: Orenha, Renato P., Parreira, Renato Luis Tame, Nagurniak, Glaucio R., Silva, Gabriel Reynald da, Piotrowski, Maurício J.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da Universidade Cruzeiro do Sul
Texto Completo: https://repositorio.cruzeirodosul.edu.br/handle/123456789/3933
https://doi.org/10.1039/D2CP00148A
Resumo: The complexity of Cu13, Ag13, and Au13 coinage-metal clusters was investigated through their energy contributions via a density functional theory study, considering improvements in the PBE functional, such as van der Waals (vdW) corrections, spin–orbit coupling (SOC), Hubbard term (+U), and their combinations. Investigating two-dimensional (planar 2D) and three-dimensional (distorted 3D, CUB – cuboctahedral, and ICO – icosahedral) configurations, we found that vdW corrections are dominant in modulating the stability swapping between 2D and ICO (3D) for Ag13 (Au13), whereas for Cu13 its role is increasing the relative stability between 2D (least stable) and 3D (most stable), setting ICO as the reference. Among the energy portions that constitute the relative total energy, the dimensionality difference correlates with the magnitude of the relative dispersion energy (large for 2D/ICO and small for 3D/ICO) as the causal factor responsible for an eventual stability swapping. For instance, empirical vdW corrections may favor Ag13 as ICO, while semi empirical ones tend to swap the stability by favoring 2D. The same tendency is observed for Au13, except when SOC is included, which enlarges the stability of 3D over 2D. Energy decomposition analysis combined with the natural orbitals for the chemical valence approach confirmed the correlations between the dimensionality difference and the magnitude of the relative dispersion energies. Our structural analysis protocol was able to capture the local distortion effects (or even their absence) through the quantification of the Hausdorff chirality measure. Here, ICO, CUB, and 2D are achiral configurations for all coinage-metal clusters, whereas Cu13 as 3D presents a slight chirality when vdW correction based on many body dispersion is used, at the same time Ag13 as 3D turned out to be chiral for all calculation protocols as evidence of the role of the chemical composition. Palavras-chave: metal clusters, Au13, Ag13, Cu13, 2D/3D stability
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spelling 2022-06-28T19:31:06Z2022-06-28T19:31:06Z2022-06-131463-9076https://repositorio.cruzeirodosul.edu.br/handle/123456789/3933https://doi.org/10.1039/D2CP00148AThe complexity of Cu13, Ag13, and Au13 coinage-metal clusters was investigated through their energy contributions via a density functional theory study, considering improvements in the PBE functional, such as van der Waals (vdW) corrections, spin–orbit coupling (SOC), Hubbard term (+U), and their combinations. Investigating two-dimensional (planar 2D) and three-dimensional (distorted 3D, CUB – cuboctahedral, and ICO – icosahedral) configurations, we found that vdW corrections are dominant in modulating the stability swapping between 2D and ICO (3D) for Ag13 (Au13), whereas for Cu13 its role is increasing the relative stability between 2D (least stable) and 3D (most stable), setting ICO as the reference. Among the energy portions that constitute the relative total energy, the dimensionality difference correlates with the magnitude of the relative dispersion energy (large for 2D/ICO and small for 3D/ICO) as the causal factor responsible for an eventual stability swapping. For instance, empirical vdW corrections may favor Ag13 as ICO, while semi empirical ones tend to swap the stability by favoring 2D. The same tendency is observed for Au13, except when SOC is included, which enlarges the stability of 3D over 2D. Energy decomposition analysis combined with the natural orbitals for the chemical valence approach confirmed the correlations between the dimensionality difference and the magnitude of the relative dispersion energies. Our structural analysis protocol was able to capture the local distortion effects (or even their absence) through the quantification of the Hausdorff chirality measure. Here, ICO, CUB, and 2D are achiral configurations for all coinage-metal clusters, whereas Cu13 as 3D presents a slight chirality when vdW correction based on many body dispersion is used, at the same time Ag13 as 3D turned out to be chiral for all calculation protocols as evidence of the role of the chemical composition. Palavras-chave: metal clusters, Au13, Ag13, Cu13, 2D/3D stabilityengUniversidade de FrancaUNIFRANBrasilPhysical Chemistry Chemical PhysicsCNPQ::CIENCIAS EXATAS E DA TERRA::QUIMICAmetal clustersAu13Ag13Cu132D/3D stabilityThe effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article241165156524Guedes-Sobrinho, DiegoOrenha, Renato P.Parreira, Renato Luis TameNagurniak, Glaucio R.Silva, Gabriel Reynald daPiotrowski, Maurício J.info:eu-repo/semantics/openAccessreponame:Repositório Institucional da Universidade Cruzeiro do Sulinstname:Universidade Cruzeiro do Sul (UNICSUL)instacron:UNICSULLICENSElicense.txtlicense.txttext/plain; charset=utf-81748http://dev.siteworks.com.br:8080/jspui/bitstream/123456789/3933/2/license.txt8a4605be74aa9ea9d79846c1fba20a33MD52123456789/39332022-06-29 13:27:12.318oai:repositorio.cruzeirodosul.edu.br: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Repositório InstitucionalPRIhttps://repositorio.cruzeirodosul.edu.br/oai/requestmary.pela@unicid.edu.bropendoar:2022-06-29T16:27:12Repositório Institucional da Universidade Cruzeiro do Sul - Universidade Cruzeiro do Sul (UNICSUL)false
dc.title.pt_BR.fl_str_mv The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
title The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
spellingShingle The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
Guedes-Sobrinho, Diego
CNPQ::CIENCIAS EXATAS E DA TERRA::QUIMICA
metal clusters
Au13
Ag13
Cu13
2D/3D stability
title_short The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
title_full The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
title_fullStr The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
title_full_unstemmed The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
title_sort The effect of different energy portions on the 2D/ 3D stability swapping for 13-atom metal clusters†
author Guedes-Sobrinho, Diego
author_facet Guedes-Sobrinho, Diego
Orenha, Renato P.
Parreira, Renato Luis Tame
Nagurniak, Glaucio R.
Silva, Gabriel Reynald da
Piotrowski, Maurício J.
author_role author
author2 Orenha, Renato P.
Parreira, Renato Luis Tame
Nagurniak, Glaucio R.
Silva, Gabriel Reynald da
Piotrowski, Maurício J.
author2_role author
author
author
author
author
dc.contributor.author.fl_str_mv Guedes-Sobrinho, Diego
Orenha, Renato P.
Parreira, Renato Luis Tame
Nagurniak, Glaucio R.
Silva, Gabriel Reynald da
Piotrowski, Maurício J.
dc.subject.cnpq.fl_str_mv CNPQ::CIENCIAS EXATAS E DA TERRA::QUIMICA
topic CNPQ::CIENCIAS EXATAS E DA TERRA::QUIMICA
metal clusters
Au13
Ag13
Cu13
2D/3D stability
dc.subject.por.fl_str_mv metal clusters
Au13
Ag13
Cu13
2D/3D stability
description The complexity of Cu13, Ag13, and Au13 coinage-metal clusters was investigated through their energy contributions via a density functional theory study, considering improvements in the PBE functional, such as van der Waals (vdW) corrections, spin–orbit coupling (SOC), Hubbard term (+U), and their combinations. Investigating two-dimensional (planar 2D) and three-dimensional (distorted 3D, CUB – cuboctahedral, and ICO – icosahedral) configurations, we found that vdW corrections are dominant in modulating the stability swapping between 2D and ICO (3D) for Ag13 (Au13), whereas for Cu13 its role is increasing the relative stability between 2D (least stable) and 3D (most stable), setting ICO as the reference. Among the energy portions that constitute the relative total energy, the dimensionality difference correlates with the magnitude of the relative dispersion energy (large for 2D/ICO and small for 3D/ICO) as the causal factor responsible for an eventual stability swapping. For instance, empirical vdW corrections may favor Ag13 as ICO, while semi empirical ones tend to swap the stability by favoring 2D. The same tendency is observed for Au13, except when SOC is included, which enlarges the stability of 3D over 2D. Energy decomposition analysis combined with the natural orbitals for the chemical valence approach confirmed the correlations between the dimensionality difference and the magnitude of the relative dispersion energies. Our structural analysis protocol was able to capture the local distortion effects (or even their absence) through the quantification of the Hausdorff chirality measure. Here, ICO, CUB, and 2D are achiral configurations for all coinage-metal clusters, whereas Cu13 as 3D presents a slight chirality when vdW correction based on many body dispersion is used, at the same time Ag13 as 3D turned out to be chiral for all calculation protocols as evidence of the role of the chemical composition. Palavras-chave: metal clusters, Au13, Ag13, Cu13, 2D/3D stability
publishDate 2022
dc.date.accessioned.fl_str_mv 2022-06-28T19:31:06Z
dc.date.available.fl_str_mv 2022-06-28T19:31:06Z
dc.date.issued.fl_str_mv 2022-06-13
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv https://repositorio.cruzeirodosul.edu.br/handle/123456789/3933
dc.identifier.issn.pt_BR.fl_str_mv 1463-9076
dc.identifier.doi.pt_BR.fl_str_mv https://doi.org/10.1039/D2CP00148A
identifier_str_mv 1463-9076
url https://repositorio.cruzeirodosul.edu.br/handle/123456789/3933
https://doi.org/10.1039/D2CP00148A
dc.language.iso.fl_str_mv eng
language eng
dc.relation.ispartof.pt_BR.fl_str_mv Physical Chemistry Chemical Physics
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv Universidade de Franca
dc.publisher.initials.fl_str_mv UNIFRAN
dc.publisher.country.fl_str_mv Brasil
publisher.none.fl_str_mv Universidade de Franca
dc.source.none.fl_str_mv reponame:Repositório Institucional da Universidade Cruzeiro do Sul
instname:Universidade Cruzeiro do Sul (UNICSUL)
instacron:UNICSUL
instname_str Universidade Cruzeiro do Sul (UNICSUL)
instacron_str UNICSUL
institution UNICSUL
reponame_str Repositório Institucional da Universidade Cruzeiro do Sul
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repository.name.fl_str_mv Repositório Institucional da Universidade Cruzeiro do Sul - Universidade Cruzeiro do Sul (UNICSUL)
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