Radiative defects in GaN nanocolumns: Correlation with growth conditions and sample morphology
Creators
- 1. Instituto de Sistemas Optoelectronicos y Microtecnologia, Universidad Politecnica de Madrid, Ciudad Universitaria s/n, 28040 Madrid (Spain)
Description
Low-temperature photoluminescence is studied in detail in GaN nanocolumns (NCs) grown by plasma-assisted molecular beam epitaxy under various conditions (substrate temperature and impinging Ga/N flux ratio). The relative intensities of the different emission lines, in particular those related to structural defects, appear to be correlated with the growth conditions, and clearly linked to the NC sample morphology. We demonstrate, in particular, that all lines comprised between 3.10 and 3.42 eV rapidly lose intensity when the growth conditions are such that the NC coalescence is reduced. The well-known line around 3.45 eV, characteristic of GaN NC samples, shows, however, a behavior that is exactly the opposite of the other lines, namely, for growth conditions leading to reduced NC coalescence, this line tends to become more prominent, thus proving to be intrinsic to individual GaN NCs.
Additional details
Identifiers
- DOI
- 10.1063/1.3556643;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 98
- Journal Issue
- 8
- Journal Page Range
- p. 083104-083104.3
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42108943
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- COALESCENCE; CORRELATIONS; CRYSTAL DEFECTS; CRYSTAL GROWTH; GALLIUM NITRIDES; MOLECULAR BEAM EPITAXY; NANOSTRUCTURES; PHOTOLUMINESCENCE; PLASMA; SEMICONDUCTOR MATERIALS; SUBSTRATES
- Descriptors DEC
- CRYSTAL GROWTH METHODS; CRYSTAL STRUCTURE; EMISSION; EPITAXY; GALLIUM COMPOUNDS; LUMINESCENCE; MATERIALS; NITRIDES; NITROGEN COMPOUNDS; PHOTON EMISSION; PNICTIDES
Optional Information
- Notes
- (c) 2011 American Institute of Physics