File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

Conference Paper: 3-D atomistic kinetic Monte Carlo simulations of point defect incorporation during CVD diamond film growth

Title3-D atomistic kinetic Monte Carlo simulations of point defect incorporation during CVD diamond film growth
Authors
Issue Date1996
Citation
Materials Research Society Symposium - Proceedings, 1996, v. 441, p. 509-514 How to Cite?
AbstractThe incorporation of vacancies and H atoms into {100}- and {111}-oriented diamond films during CVD growth in an atmosphere of H, H2, CH3, and C2H2 is simulated atomistically. The growing films are represented in three dimensions by a diamond cubic lattice, and the temporal evolution of the surfaces is accomplished by a kinetic Monte Carlo method. The dimer bonding of diamond atoms on the {100} surface is treated explicitly. Growth begins on {100}(2×1):H and {111}:H surfaces containing 288 and 300 atoms, respectively, in the surface plane, and the growth of approximately sixty atomic layers (18,000 atoms) is accomplished at each of fifteen substrate temperatures between 800 and 1500 K. The growth rates depend on the combined contributions to growth from CH3 and C2H2, whereas the point defect concentrations depend on the ratio of C2H2 to CH3 growth. The maximum {100} growth rate is achieved at approximately 1200 K. Point defect concentrations are low at temperatures below 1300 K, but become high above 1300 K. Growth efficiency, defined as the ratio of growth rate to defect concentration, is maximum for both film orientations at substrate temperatures in the vicinity of 1100 to 1200 K.
Persistent Identifierhttp://hdl.handle.net/10722/303154
ISSN
2019 SCImago Journal Rankings: 0.114

 

DC FieldValueLanguage
dc.contributor.authorBattaile, C.-
dc.contributor.authorSrolovitz, D. J.-
dc.contributor.authorButler, J. E.-
dc.date.accessioned2021-09-15T08:24:44Z-
dc.date.available2021-09-15T08:24:44Z-
dc.date.issued1996-
dc.identifier.citationMaterials Research Society Symposium - Proceedings, 1996, v. 441, p. 509-514-
dc.identifier.issn0272-9172-
dc.identifier.urihttp://hdl.handle.net/10722/303154-
dc.description.abstractThe incorporation of vacancies and H atoms into {100}- and {111}-oriented diamond films during CVD growth in an atmosphere of H, H2, CH3, and C2H2 is simulated atomistically. The growing films are represented in three dimensions by a diamond cubic lattice, and the temporal evolution of the surfaces is accomplished by a kinetic Monte Carlo method. The dimer bonding of diamond atoms on the {100} surface is treated explicitly. Growth begins on {100}(2×1):H and {111}:H surfaces containing 288 and 300 atoms, respectively, in the surface plane, and the growth of approximately sixty atomic layers (18,000 atoms) is accomplished at each of fifteen substrate temperatures between 800 and 1500 K. The growth rates depend on the combined contributions to growth from CH3 and C2H2, whereas the point defect concentrations depend on the ratio of C2H2 to CH3 growth. The maximum {100} growth rate is achieved at approximately 1200 K. Point defect concentrations are low at temperatures below 1300 K, but become high above 1300 K. Growth efficiency, defined as the ratio of growth rate to defect concentration, is maximum for both film orientations at substrate temperatures in the vicinity of 1100 to 1200 K.-
dc.languageeng-
dc.relation.ispartofMaterials Research Society Symposium - Proceedings-
dc.title3-D atomistic kinetic Monte Carlo simulations of point defect incorporation during CVD diamond film growth-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1557/PROC-441-509-
dc.identifier.scopuseid_2-s2.0-0030658525-
dc.identifier.volume441-
dc.identifier.spage509-
dc.identifier.epage514-

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats