Abstract
GaAsSbN was grown by organometallic vapor phase epitaxy (OMVPE) as an alternative material to InGaAsN for long wavelength emission on GaAs substrates. OMVPE of GaAsSbN using trimethylgallium, 100% arsine, trimethylantimony, and 1,1-dimethylhydrazine was found to be kinetically limited at growth temperatures ranging from 520°C to 600°C, with an activation energy of 10.4kcal/mol. The growth rate was linearly dependent on the group III flow and has a complex dependence on the group V constituents. A room temperature photoluminescence wavelength of > 1.3 μm was observed for unannealed GaAs0.69Sb0.3N0.01. Low temperature (4K) photoluminescence of GaAs0.69Sb0.3N0.01 shows an increase in FWHM of 2.4-3.4 times the FWHM of GaAs0.7Sb 0.3, a red shift of 55-77meV, and a decrease in intensity of one to two orders of magnitude. Hall measurements indicate a behavior similar to that of InGaAsN, a 300K hole mobility of 350cm2/V-s with a 1.0 × 1017/cm3 background hole concentration, and a 77K mobility of 1220cm2/V-s with a background hole concentration of 4.8 × 1016/cm3. The hole mass of GaAs 0.7Sb0.3/GaAs heterostructures was estimated at 0.37-0.40mo, and we estimate an electron mass of 0.2-0.3m o for the GaAs0.69Sb0.3N0.01/GaAs system. The reduced exciton mass for GaAsSbN was estimated at about twice that found for GaAsSb by a comparison of diamagnetic shift vs. magnetic field. © 2003 Elsevier B.V. All rights reserved.
| Original language | English |
|---|---|
| Title of host publication | Journal of Crystal Growth |
| Pages | 398-403 |
| Number of pages | 6 |
| Volume | 261 |
| Edition | 2-3 |
| DOIs | |
| State | Published - Jan 19 2004 |
| Externally published | Yes |
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