Abstrakt
The energy distribution of the surface state density NSS(E) on the n-type InP surface was determined from a rigorous computer analysis of the dependence of the band-to-band photoluminescence efficiency (YPL) versus excitation light intensity (Φ). The analysed experimental YPL-Φ spectrum, taken from the literature, was obtained at room temperature for the chemically polished n-InP100 surface. The theoretical values of YPL were calculated using a numerical simulator, taking account of all possible bulk and surface recombination processes. We reproduced very well the experimental YPL-Φ dependence, which exhibited a strong increase of YPL. We also determined the continuous U-shaped NSS(E) distribution from the best fit to the experimental data by applying a novel fully-computer procedure based on genetic algorithm. Furthermore, we found that the surface non-radiative recombination dominates over the bulk recombination channels (in terms of recombination rates), and governs the behaviour of radiative recombination versus Φ.
| Język oryginału | angielski |
|---|---|
| Strony (od–do) | 240-244 |
| Liczba stron | 5 |
| Czasopismo | Surface Science |
| Tom | 507-510 |
| Identyfikatory DOI | |
| Status publikacji | Opublikowano - cze 2002 |
Obszary tematyczne ASJC Scopus
- Fizyka materii skondensowanej
- Powierzchnie i interfejsy
- Powierzchnie, powłoki i filmy
- Chemia materiałowa
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