Published June 13, 2005
| Version v1
Journal article
Effect of annealing temperature ramp rate on bubble formation in helium-implanted silicon
Creators
- 1. Department of Physics and Astronomy, University of Western Ontario, London, Ontario, N6A3K7 (Canada)
Description
We have implanted 3He into Si(100) at 1.0 MeV ion energy and to fluences ranging between 2x1015 and 2x1016 cm-2, followed by annealing at 700 deg. C. Heating ramp rates have been systematically varied over more than two decades (0.3 deg. C/s to 100 deg. C/s) at each fluence. The retention of 3He is measured through the 3He(d,p)4He nuclear reaction yield. We show that gas retention can be varied by more than an order of magnitude even while the other anneal parameters--anneal temperature and anneal time--are maintained constant. Cross-sectional scanning electron micrographs confirm the presence of planetarylike cavity structures at a depth closely matching that calculated for the damage peak
Additional details
Identifiers
- DOI
- 10.1063/1.1947384;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 86
- Journal Issue
- 24
- Journal Page Range
- p. 241907-241907.3
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37017584
- Subject category
- S36: MATERIALS SCIENCE;
- Descriptors DEI
- ANNEALING; BUBBLES; DEUTERON REACTIONS; HEATING; HELIUM 3; HELIUM 3 TARGET; HELIUM 4; HELIUM IONS; ION IMPLANTATION; MEV RANGE 01-10; NUCLEAR REACTION YIELD; PROTONS; SCANNING ELECTRON MICROSCOPY; SEMICONDUCTOR MATERIALS; SILICON
- Descriptors DEC
- BARYONS; CHARGED PARTICLES; CHARGED-PARTICLE REACTIONS; ELECTRON MICROSCOPY; ELEMENTARY PARTICLES; ELEMENTS; ENERGY RANGE; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; FERMIONS; HADRONS; HEAT TREATMENTS; HELIUM ISOTOPES; IONS; ISOTOPES; LIGHT NUCLEI; MATERIALS; MEV RANGE; MICROSCOPY; NUCLEAR REACTIONS; NUCLEI; NUCLEONS; SEMIMETALS; STABLE ISOTOPES; TARGETS; YIELDS
Optional Information
- Notes
- (c) 2005 American Institute of Physics