Nearest-neighbor configuration in (GaIn)(NAs) probed by X-ray absorption spectroscopy
Creators
- 1. Solid State and Photonics Laboratory, Stanford University, Stanford, California 94305 (United States)
- 2. Lawrence Berkeley National Laboratory, Berkeley, California 94720 (United States)
- 3. Matsushita Electric Industrial Co., Ltd., Osaka (Japan)
- 4. Wakayama University, Wakayama (Japan)
Description
Ga1-xInxNyAs1-y is a promising material system for the fabrication of inexpensive 'last-mile' optoelectronic components. However, details of its atomic arrangement and the relationship to observed optical properties is not fully known. Particularly, a blueshift of emission wavelength is observed after annealing. In this work, we use x-ray absorption fine structure to study the chemical environment around N atoms in the material before and after annealing. We find that as-grown molecular beam epitaxy material consists of a nearly random distribution of atoms, while postannealed material shows segregation of In toward N. Ab initio simulations show that this short-range ordering creates a more thermodynamically stable alloy and is responsible for blueshifting the emission
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 90
- Journal Issue
- 14
- Journal Page Range
- p. 145505-145505.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35041524
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- ABSORPTION SPECTROSCOPY; ANNEALING; DENSITY FUNCTIONAL METHOD; FINE STRUCTURE; GALLIUM ARSENIDES; INDIUM COMPOUNDS; MOLECULAR BEAM EPITAXY; NITROGEN COMPOUNDS; SIMULATION; X-RAY SPECTROSCOPY
- Descriptors DEC
- ARSENIC COMPOUNDS; ARSENIDES; CALCULATION METHODS; CRYSTAL GROWTH METHODS; EPITAXY; GALLIUM COMPOUNDS; HEAT TREATMENTS; PNICTIDES; SPECTROSCOPY; VARIATIONAL METHODS
Optional Information
- Notes
- (c) 2003 The American Physical Society