OMVPE of GaAsSbN for long wavelength emission on GaAs

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 temp...

Full description

Saved in:
Bibliographic Details
Published in:Journal of crystal growth Vol. 261; no. 2; pp. 398 - 403
Main Authors: Peake, G.M., Waldrip, K.E., Hargett, T.W., Modine, N.A., Serkland, D.K.
Format: Journal Article Conference Proceeding
Language:English
Published: Amsterdam Elsevier B.V 19-01-2004
Elsevier
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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 10.4 kcal/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 GaAs 0.69Sb 0.3N 0.01. Low temperature (4 K) photoluminescence of GaAs 0.69Sb 0.3N 0.01 shows an increase in FWHM of 2.4–3.4 times the FWHM of GaAs 0.7Sb 0.3, a red shift of 55–77 meV, and a decrease in intensity of one to two orders of magnitude. Hall measurements indicate a behavior similar to that of InGaAsN, a 300 K hole mobility of 350 cm 2/V-s with a 1.0×10 17/cm 3 background hole concentration, and a 77 K mobility of 1220 cm 2/V-s with a background hole concentration of 4.8×10 16/cm 3. The hole mass of GaAs 0.7Sb 0.3/GaAs heterostructures was estimated at 0.37–0.40 m o, and we estimate an electron mass of 0.2–0.3 m o for the GaAs 0.69Sb 0.3N 0.01/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.
Bibliography:ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0022-0248
1873-5002
DOI:10.1016/j.jcrysgro.2003.11.034