Nanoscale anglesite growth on the celestite (001) face.
In situ atomic force microscopy (AFM) was used to study the growth behaviour of anglesite (PbSO4) monolayers on the celestite (001) face. Growth was promoted by exposing the celestite cleavage surfaces to aqueous solutions that were supersaturated with respect to anglesite. The solution supersaturat...
| Autores: | , |
|---|---|
| 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:20.500.14352/43641 |
| Acceso en línea: | https://hdl.handle.net/20.500.14352/43641 |
| Access Level: | acceso abierto |
| Palabra clave: | 549.76 548.2 539.2 Surface topography Atomic force microscopy Crystal Growth Epitaxy Aqueous solutions Solid–liquid interfaces Celestite Anglesite Cristalografía (Geología) Mineralogía (Geología) 2506.11 Mineralogía |
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Nanoscale anglesite growth on the celestite (001) face.Pina Martínez, Carlos ManuelRico García, Aida549.76548.2539.2Surface topographyAtomic force microscopyCrystal Growth EpitaxyAqueous solutionsSolid–liquid interfacesCelestiteAnglesiteCristalografía (Geología)Mineralogía (Geología)2506.11 MineralogíaIn situ atomic force microscopy (AFM) was used to study the growth behaviour of anglesite (PbSO4) monolayers on the celestite (001) face. Growth was promoted by exposing the celestite cleavage surfaces to aqueous solutions that were supersaturated with respect to anglesite. The solution supersaturation, βang, was varied from 1.05 to 3.09 (where βang = a(Pb2+)•a(SO42-)/Ksp,ang). In this range of supersaturation, two single anglesite monolayers (~3.5 Å in height each) from pre-existent celestite steps were grown. However, for solution supersaturation of the values of βang < 1.89 +- 0.06, subsequent multilayer growth is strongly inhibited. AFM observations indicate that the inhibition of a continuous layer-by-layer growth of anglesite on the celestite (001) face is due to the in-plane strain generated by the slight difference between the anglesite and celestite lattice parameters (i.e. the linear misfits are lower than 1.1%). The minimum supersaturation required to overcome the energy barrier for multilayer growth gave an estimate of the in-plane strain energy: 11.4 +/- 0.6 mJ/m2. Once this energy barrier is overcome, a multilayer Frank–van der Merwe epitaxial growth was observed.ElsevierUniversidad Complutense de Madrid20092009-09-0120092009-09-01journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/43641reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/436412026-06-02T12:44:21Z |
| dc.title.none.fl_str_mv |
Nanoscale anglesite growth on the celestite (001) face. |
| title |
Nanoscale anglesite growth on the celestite (001) face. |
| spellingShingle |
Nanoscale anglesite growth on the celestite (001) face. Pina Martínez, Carlos Manuel 549.76 548.2 539.2 Surface topography Atomic force microscopy Crystal Growth Epitaxy Aqueous solutions Solid–liquid interfaces Celestite Anglesite Cristalografía (Geología) Mineralogía (Geología) 2506.11 Mineralogía |
| title_short |
Nanoscale anglesite growth on the celestite (001) face. |
| title_full |
Nanoscale anglesite growth on the celestite (001) face. |
| title_fullStr |
Nanoscale anglesite growth on the celestite (001) face. |
| title_full_unstemmed |
Nanoscale anglesite growth on the celestite (001) face. |
| title_sort |
Nanoscale anglesite growth on the celestite (001) face. |
| dc.creator.none.fl_str_mv |
Pina Martínez, Carlos Manuel Rico García, Aida |
| author |
Pina Martínez, Carlos Manuel |
| author_facet |
Pina Martínez, Carlos Manuel Rico García, Aida |
| author_role |
author |
| author2 |
Rico García, Aida |
| author2_role |
author |
| dc.contributor.none.fl_str_mv |
Universidad Complutense de Madrid |
| dc.subject.none.fl_str_mv |
549.76 548.2 539.2 Surface topography Atomic force microscopy Crystal Growth Epitaxy Aqueous solutions Solid–liquid interfaces Celestite Anglesite Cristalografía (Geología) Mineralogía (Geología) 2506.11 Mineralogía |
| topic |
549.76 548.2 539.2 Surface topography Atomic force microscopy Crystal Growth Epitaxy Aqueous solutions Solid–liquid interfaces Celestite Anglesite Cristalografía (Geología) Mineralogía (Geología) 2506.11 Mineralogía |
| description |
In situ atomic force microscopy (AFM) was used to study the growth behaviour of anglesite (PbSO4) monolayers on the celestite (001) face. Growth was promoted by exposing the celestite cleavage surfaces to aqueous solutions that were supersaturated with respect to anglesite. The solution supersaturation, βang, was varied from 1.05 to 3.09 (where βang = a(Pb2+)•a(SO42-)/Ksp,ang). In this range of supersaturation, two single anglesite monolayers (~3.5 Å in height each) from pre-existent celestite steps were grown. However, for solution supersaturation of the values of βang < 1.89 +- 0.06, subsequent multilayer growth is strongly inhibited. AFM observations indicate that the inhibition of a continuous layer-by-layer growth of anglesite on the celestite (001) face is due to the in-plane strain generated by the slight difference between the anglesite and celestite lattice parameters (i.e. the linear misfits are lower than 1.1%). The minimum supersaturation required to overcome the energy barrier for multilayer growth gave an estimate of the in-plane strain energy: 11.4 +/- 0.6 mJ/m2. Once this energy barrier is overcome, a multilayer Frank–van der Merwe epitaxial growth was observed. |
| publishDate |
2009 |
| dc.date.none.fl_str_mv |
2009 2009-09-01 2009 2009-09-01 |
| 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/20.500.14352/43641 |
| url |
https://hdl.handle.net/20.500.14352/43641 |
| 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 |
Elsevier |
| publisher.none.fl_str_mv |
Elsevier |
| 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 |
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1869420043847073792 |
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15.300724 |