Published August 9, 2010
| Version v1
Journal article
Surface-plasmon enhancement of band gap emission from ZnCdO thin films by gold particles
- 1. Division of Physics and Applied Physics, School of Physical and Mathematical Sciences, Nanyang Technological University, Singapore 637371 (Singapore)
- 2. Institute of Materials Research and Engineering, Singapore 117602 (Singapore)
Description
We present our study of the dependence of surface plasmon (SP) coupled band gap emission and defect emission on the sputtering time of gold particles on ZnCdO films. Eightfold enhancement of the band gap emission from ZnCdO thin films coated with Au particles is observed, while the defect emission is completely suppressed. The remarkable enhancement of the band gap emission is mainly attributed to the coupling between excitons in ZnCdO films and the SP of Au particles. While the suppression of the defect emission may be ascribed to a combined effect of the reduction in surface defects and the charge transfer from defect level to the Au Fermi level.
Additional details
Identifiers
- DOI
- 10.1063/1.3476357;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 97
- Journal Issue
- 6
- Journal Page Range
- p. 061104-061104.3
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42060551
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S36: MATERIALS SCIENCE;
- Descriptors DEI
- CADMIUM OXIDES; CHARGE EXCHANGE; COATINGS; COUPLING; CRYSTAL DEFECTS; ELECTRONIC STRUCTURE; ENERGY GAP; EXCITONS; FERMI LEVEL; GOLD; PARTICLES; PHOTOLUMINESCENCE; PLASMONS; SEMICONDUCTOR MATERIALS; SPUTTERING; SURFACES; THIN FILMS; ZINC COMPOUNDS
- Descriptors DEC
- CADMIUM COMPOUNDS; CHALCOGENIDES; CRYSTAL STRUCTURE; ELEMENTS; EMISSION; ENERGY LEVELS; FILMS; LUMINESCENCE; MATERIALS; METALS; OXIDES; OXYGEN COMPOUNDS; PHOTON EMISSION; QUASI PARTICLES; TRANSITION ELEMENTS
Optional Information
- Notes
- (c) 2010 American Institute of Physics