Sub-band-gap absorption in Ga2O3
Abstract
β-Ga2O3 is a transparent conducting oxide that, due to its large bandgap of 4.8 eV, exhibits transparency into the UV. However, the free carriers that enable the conductivity can absorb light. We study the effect of free carriers on the properties of Ga2O3 using hybrid density functional theory. The presence of free carriers leads to sub-band-gap absorption and a Burstein-Moss shift in the onset of absorption. We find that for a concentration of 1020 carriers, the Fermi level is located 0.23 eV above the conduction-band minimum. This leads to an increase in the electron effective mass from 0.27–0.28 me to 0.35–0.37 me and a sub-band-gap absorption band with a peak value of 0.6 × 103 cm–1 at 3.37 eV for light polarized along the x or z direction. Both across-the-gap and free-carrier absorption depend strongly on the polarization of the incoming light. We also provide parametrizations of the conduction-band shape and the effective mass as a function of the Fermi level. β-Ga2O3 exhibits very good electronic conductivity in spite of its bandgap of 4.8 eV; this large gap makes it transparent into the UV. This combination allows for applications in devices such as deep-UV blind detectors and contacts for solarmore »
- Authors:
-
- Univ. of California, Santa Barbara, CA (United States)
- Publication Date:
- Research Org.:
- Univ. of California, Santa Barbara, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Basic Energy Sciences (BES)
- OSTI Identifier:
- 1505556
- Alternate Identifier(s):
- OSTI ID: 1408160
- Grant/Contract Number:
- SC0010689
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Applied Physics Letters
- Additional Journal Information:
- Journal Volume: 111; Journal Issue: 18; Journal ID: ISSN 0003-6951
- Publisher:
- American Institute of Physics (AIP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 36 MATERIALS SCIENCE
Citation Formats
Peelaers, Hartwin, and Van de Walle, Chris G. Sub-band-gap absorption in Ga2O3. United States: N. p., 2017.
Web. doi:10.1063/1.5001323.
Peelaers, Hartwin, & Van de Walle, Chris G. Sub-band-gap absorption in Ga2O3. United States. https://doi.org/10.1063/1.5001323
Peelaers, Hartwin, and Van de Walle, Chris G. Fri .
"Sub-band-gap absorption in Ga2O3". United States. https://doi.org/10.1063/1.5001323. https://www.osti.gov/servlets/purl/1505556.
@article{osti_1505556,
title = {Sub-band-gap absorption in Ga2O3},
author = {Peelaers, Hartwin and Van de Walle, Chris G.},
abstractNote = {β-Ga2O3 is a transparent conducting oxide that, due to its large bandgap of 4.8 eV, exhibits transparency into the UV. However, the free carriers that enable the conductivity can absorb light. We study the effect of free carriers on the properties of Ga2O3 using hybrid density functional theory. The presence of free carriers leads to sub-band-gap absorption and a Burstein-Moss shift in the onset of absorption. We find that for a concentration of 1020 carriers, the Fermi level is located 0.23 eV above the conduction-band minimum. This leads to an increase in the electron effective mass from 0.27–0.28 me to 0.35–0.37 me and a sub-band-gap absorption band with a peak value of 0.6 × 103 cm–1 at 3.37 eV for light polarized along the x or z direction. Both across-the-gap and free-carrier absorption depend strongly on the polarization of the incoming light. We also provide parametrizations of the conduction-band shape and the effective mass as a function of the Fermi level. β-Ga2O3 exhibits very good electronic conductivity in spite of its bandgap of 4.8 eV; this large gap makes it transparent into the UV. This combination allows for applications in devices such as deep-UV blind detectors and contacts for solar cells. It also enables high-power devices, such as high-voltage metal-semiconductor field-effect transistors and Schottky barrier diodes.},
doi = {10.1063/1.5001323},
journal = {Applied Physics Letters},
number = 18,
volume = 111,
place = {United States},
year = {Fri Nov 03 00:00:00 EDT 2017},
month = {Fri Nov 03 00:00:00 EDT 2017}
}
Web of Science
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