2011
DOI: 10.1002/pssc.201000956
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GaInN quantum well design and measurement conditions affecting the emission energy S‐shape

Abstract: Polarization fields and charge carrier localization are the dominant factors defining the radiative recombination processes in the quantum wells of most AlGaInN‐based optoelectronic devices. Both factors determine emission energy, emission line width, recombination times, and internal quantum efficiency. For a deeper understanding of the charge carrier recombination processes, we have performed temperature and excitation power dependent photoluminescence experiments on epitaxially grown GaInN structures to stu… Show more

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Cited by 7 publications
(11 citation statements)
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“…The turning points are at higher temperature when the indium mol fraction is increased (first turning point temperatures listed in table 1). These features point strongly to charge carrier localization effects [29][30][31]. The emission energy 'S-shape' behavior is not as pronounced as in most c-plane GaInN quantum well structures (e.g.…”
Section: Evidence For Strong Localizationmentioning
confidence: 93%
“…The turning points are at higher temperature when the indium mol fraction is increased (first turning point temperatures listed in table 1). These features point strongly to charge carrier localization effects [29][30][31]. The emission energy 'S-shape' behavior is not as pronounced as in most c-plane GaInN quantum well structures (e.g.…”
Section: Evidence For Strong Localizationmentioning
confidence: 93%
“…Thus, when the localization degree is increased, peak wavelength features a stronger red‐shift and the S‐shaped curve moves to higher temperatures. Gaussian band‐tail model: Etrue(Ttrue)=Etrue(0true)αT2/true(β+Ttrue)σ2/kBT can be applied to fit the “S”‐shaped curve , where E (0) is the transition energy at 0 K, α, and β are known as Varshni thermal coefficients, and broadening factor σ represents the localization degree. The fitting results and the parameters are shown in Fig.…”
Section: Resultsmentioning
confidence: 99%
“…The absorbed pump power density was determined from the measured incident power density by utilizing the absorption coefficient extrapolated to 380 nm from the measured optical gain spectra using a model fit. As the excitation takes place close to the quantum well band edge, this procedure takes into account the strong change of absorption due to band filling [9]. Moreover, the waveguide loss was determined from the low energy tail of the gain spectra [10].…”
Section: Measurements and Resultsmentioning
confidence: 99%