Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3458
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dc.creatorVivas P. G.-
dc.creatorSilva E. E. da-
dc.creatorCarvalho L. C. de-
dc.creatorAlves J. L. A.-
dc.creatorAlves H. W. Leite-
dc.creatorScolfaro L. M. R.-
dc.creatorLeite J. R.-
dc.date2002-
dc.date.accessioned2013-05-30T01:59:35Z-
dc.date.available2013-05-30T01:59:35Z-
dc.date.issued2013-05-30-
dc.identifierhttp://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332002000200042-
dc.identifierhttp://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2002&volume=32&issue=2a&spage=396-
dc.identifier.urihttp://koha.mediu.edu.my:8181/jspui/handle/123456789/3458-
dc.descriptionIn this work, using Density Functional, Hartree-Fock and Extended Hückel Theories together with the supercell and cluster model approaches, we present our preliminary results for the simulation of the adsorption of Si and C atoms over the (111) SiC surfaces as well as the torsion of SiC molecules at that surfaces. Our results shown that, before and after the adsorption, the cubic structure are the most stable one, when compared with the hexagonal ones. However, the torsional energy barrier between the cubic and the hexagonal structures is small enough that, at the conditions of SiC growth, it facilitates the SiC polytype formation.-
dc.publisherSociedade Brasileira de Física-
dc.sourceBrazilian Journal of Physics-
dc.titleAdsorption of Si and C atoms over SiC (111) surfaces-
Appears in Collections:Physics and Astronomy

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