Published June 30, 2005
| Version v1
Journal article
Photoluminescence Properties of Ultra-high-quality ZnO Thin Films Grown by Sputtering Deposition
Creators
- 1. Department of Applied Physics, Graduate School of Engineering, Osaka City University (Japan)
Description
We have investigated photoluminescence properties of ultra-high quality ZnO thin films grown by an rf-magnetron sputtering method. From the results of x-ray diffraction patterns, we have found that a high growth temperature of ∼600 degree sign C and the introduction of a low-temperature buffer layer are essential in the growth of the high-quality thin films. In photoluminescence (PL) spectra, the free exciton band is observed and the defect-related PL is negligibly weak, reflecting high crystallinity of the film. Furthermore, under high-density excitation conditions, a PL band due to an exciton-exciton scattering process, the so-called P emission, is observed
Additional details
Identifiers
- DOI
- 10.1063/1.1994065;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 772
- Journal Issue
- 1
- Journal Page Range
- p. 205-206
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 27. international conference on the physics of semiconductors
- Acronym
- ICPS-27
- Dates
- 26-30 Jul 2004
- Place
- Flagstaff, AZ (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37031351
- Subject category
- S36: MATERIALS SCIENCE;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CRYSTAL GROWTH; DEPOSITION; EXCITATION; EXCITONS; LAYERS; PHOTOLUMINESCENCE; SEMICONDUCTOR MATERIALS; SPUTTERING; TEMPERATURE RANGE 0400-1000 K; THIN FILMS; X-RAY DIFFRACTION; ZINC OXIDES
- Descriptors DEC
- CHALCOGENIDES; COHERENT SCATTERING; DIFFRACTION; EMISSION; ENERGY-LEVEL TRANSITIONS; FILMS; LUMINESCENCE; MATERIALS; OXIDES; OXYGEN COMPOUNDS; PHOTON EMISSION; QUASI PARTICLES; SCATTERING; TEMPERATURE RANGE; ZINC COMPOUNDS
Optional Information
- Notes
- (c) 2005 American Institute of Physics