Journal article
Band structure engineering of superlattice-based short-, mid-, and long-wavelength infrared avalanche photodiodes for improved impact ionization rates
Journal of applied physics, Vol.92(7), pp.3771-3777
10/01/2002
DOI: 10.1063/1.1503390
Abstract
We study the effects of the electronic band structure on the hole- and electron-initiated impact ionization in Sb-based superlattice avalanche photodiodes. Earlier calculations have revealed that bulk alloy AlGaSb avalanche photodiodes with alloy composition near the resonance between the energy gap and the spin-orbit splitting have an enhanced hole to electron impact ionization coefficient ratio for a low electric field but not for a high electric field. The absence of an enhancement under high fields is due to carrier heating spreading the hole distribution in the splitoff band. A strategy to extend this type of enhancement to high fields in a superlattice involves band engineering the superlattice to place flat bands at approximately one energy gap below the top of the valence band. This prevents holes from spreading in energy and hence gives rise to strong hole-initiated impact ionization. Quantitative results are presented for short-infrared AlAs/InGaAs/AlAs/InGaSb, midinfrared InAs/InGaSb/AlSb, and long-infrared InAs/InGaSb/AlSb superlattices. (C) 2002 American Institute of Physics.
Details
- Title: Subtitle
- Band structure engineering of superlattice-based short-, mid-, and long-wavelength infrared avalanche photodiodes for improved impact ionization rates
- Creators
- K A El-RubC H Grein - University of Illinois at ChicagoM E Flatte - Harvard UniversityH Ehrenreich - Jordan University of Science and Technology
- Resource Type
- Journal article
- Publication Details
- Journal of applied physics, Vol.92(7), pp.3771-3777
- Publisher
- Amer Inst Physics
- DOI
- 10.1063/1.1503390
- ISSN
- 0021-8979
- eISSN
- 1089-7550
- Number of pages
- 7
- Language
- English
- Date published
- 10/01/2002
- Academic Unit
- Electrical and Computer Engineering; Physics and Astronomy
- Record Identifier
- 9984428819302771
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