File Download
There are no files associated with this item.
Links for fulltext
(May Require Subscription)
- Publisher Website: 10.1103/PhysRevLett.60.424
- Scopus: eid_2-s2.0-4243123805
- WOS: WOS:A1988L864500011
- Find via
Supplementary
- Citations:
- Appears in Collections:
Article: Columnar growth in thin films
Title | Columnar growth in thin films |
---|---|
Authors | |
Issue Date | 1988 |
Citation | Physical Review Letters, 1988, v. 60, n. 5, p. 424-427 How to Cite? |
Abstract | A theory for the growth of columnar microstructures in thin films is presented. The zone-I to zone-II transition temperature is predicted. The surface morphology and the columnar grain structure are obtained both analytically and numerically, and the scaling behavior of the columnar grain size with film thickness is derived. Monte Carlo simulations are used to follow the evolution of the three-dimensional zone-II microsctuctures and to account for the formation of film texture. These results agree with experimental observations. © 1988 The American Physical Society. |
Persistent Identifier | http://hdl.handle.net/10722/303328 |
ISSN | 2023 Impact Factor: 8.1 2023 SCImago Journal Rankings: 3.040 |
ISI Accession Number ID | |
Errata |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Mazor, A. | - |
dc.contributor.author | Srolovitz, D. J. | - |
dc.contributor.author | Hagan, P. S. | - |
dc.contributor.author | Bukiet, B. G. | - |
dc.date.accessioned | 2021-09-15T08:25:05Z | - |
dc.date.available | 2021-09-15T08:25:05Z | - |
dc.date.issued | 1988 | - |
dc.identifier.citation | Physical Review Letters, 1988, v. 60, n. 5, p. 424-427 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | http://hdl.handle.net/10722/303328 | - |
dc.description.abstract | A theory for the growth of columnar microstructures in thin films is presented. The zone-I to zone-II transition temperature is predicted. The surface morphology and the columnar grain structure are obtained both analytically and numerically, and the scaling behavior of the columnar grain size with film thickness is derived. Monte Carlo simulations are used to follow the evolution of the three-dimensional zone-II microsctuctures and to account for the formation of film texture. These results agree with experimental observations. © 1988 The American Physical Society. | - |
dc.language | eng | - |
dc.relation.ispartof | Physical Review Letters | - |
dc.title | Columnar growth in thin films | - |
dc.type | Article | - |
dc.description.nature | link_to_subscribed_fulltext | - |
dc.identifier.doi | 10.1103/PhysRevLett.60.424 | - |
dc.identifier.scopus | eid_2-s2.0-4243123805 | - |
dc.identifier.volume | 60 | - |
dc.identifier.issue | 5 | - |
dc.identifier.spage | 424 | - |
dc.identifier.epage | 427 | - |
dc.identifier.isi | WOS:A1988L864500011 | - |
dc.relation.erratum | doi:10.1103/PhysRevLett.60.1455.3 | - |
dc.relation.erratum | eid:eid_2-s2.0-35949013875 | - |