Nanovoids in MBE-grown SiGe alloys implanted in situ with Ge+ ions
- 1. Institute of Solid State Physics, RAS, 142432, Moscow distr., Chernogolovka (Russian Federation)
- 2. Department of Physics and Astronomy, University of Aarhus, DK-8000, Aarhus C (Denmark)
Description
Spherically shaped voids, of nanometer size, are observed in molecular-beam epitaxially grown SiGe alloy layers implanted in-situ at elevated temperature with low-energy Ge ions, followed by thermal treatments. The voids are exclusively assembled in the narrow, implanted band. The voids only appear in the layers after a heat treatment at a temperature higher than 700 deg. C, and they are stable up to 900 deg. C. Arsenic ion implantation at similar conditions does not give rise to void formation but to regular interstitial dislocation loops. The nucleation stage of the voids is accompanied by a strong photoluminescence-yield enhancement in the range of 1.4-1.55 μm, originating from the strained SiGe alloy layer which contain vacancy clusters or small voids
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. B, Condensed Matter and Materials Physics
- Journal Volume
- 67
- Journal Issue
- 23
- Journal Page Range
- p. 235310-235310.7
- ISSN
- 1098-0121
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36002151
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S36: MATERIALS SCIENCE;
- Descriptors DEI
- ARSENIC IONS; DISLOCATIONS; GERMANIUM ALLOYS; GERMANIUM IONS; HEAT TREATMENTS; INTERSTITIALS; ION IMPLANTATION; LAYERS; MOLECULAR BEAM EPITAXY; MOLECULAR BEAMS; NANOSTRUCTURES; NUCLEATION; PHOTOLUMINESCENCE; SILICON ALLOYS; TEMPERATURE RANGE 0400-1000 K; VACANCIES; VOIDS
- Descriptors DEC
- ALLOYS; BEAMS; CHARGED PARTICLES; CRYSTAL DEFECTS; CRYSTAL GROWTH METHODS; CRYSTAL STRUCTURE; EMISSION; EPITAXY; IONS; LINE DEFECTS; LUMINESCENCE; PHOTON EMISSION; POINT DEFECTS; TEMPERATURE RANGE
Optional Information
- Notes
- (c) 2003 The American Physical Society