2012
DOI: 10.1103/physrevb.86.195308
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Determination of valence-band offset at cubic CdSe/ZnTe type-II heterojunctions: A combined experimental and theoretical approach

Abstract: International audienceWe present a combined experimental and theoretical approach for the determination of the low-temperature valence band offset (VBO) at CdSe/ZnTe heterojunctions with underlying zincblende crystal structure. On the experimental side, the optical transition of the type II interface allows for a precise measurement of the type II band gap. We show how the excitation-power dependent shift of this photoluminescence (PL) signal can be used for any type II system for a precise determination of th… Show more

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Cited by 25 publications
(16 citation statements)
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“…In the present case, the time-dependent spectra are plotted, on a semi-logarithmic scale, for time delays in a geometric series 30 . In such a scheme, if the PL decay were following a power law dependence on time 31,32 , the intensity maxima between two successive curves should be visually equidistant on this semi-logarithmic plot: it is not the case here, at least for times up to ≈ 25 ns, as the larger the time, the closer the spectra look, which evidences that the PL intensity peak decrease is slower than any power law, therefore slower than any exponential. For times larger than ≈ 25 ns, the data is not so clear, and a power law behaviour cannot be fully excluded.…”
Section: Time-resolved Photoluminescencementioning
confidence: 95%
“…In the present case, the time-dependent spectra are plotted, on a semi-logarithmic scale, for time delays in a geometric series 30 . In such a scheme, if the PL decay were following a power law dependence on time 31,32 , the intensity maxima between two successive curves should be visually equidistant on this semi-logarithmic plot: it is not the case here, at least for times up to ≈ 25 ns, as the larger the time, the closer the spectra look, which evidences that the PL intensity peak decrease is slower than any power law, therefore slower than any exponential. For times larger than ≈ 25 ns, the data is not so clear, and a power law behaviour cannot be fully excluded.…”
Section: Time-resolved Photoluminescencementioning
confidence: 95%
“…The importance of the choice of the band structure method in BP calculations has already been discussed in Ref. 26. It has been pointed out that a suitably parametrized empirical tight-binding model will allow for a flexible fit to a large parameter space; the input parameters can then be either chosen from experiments or from results of more sophisticated calculation schemes.…”
Section: B Empirical Tight-binding Modelmentioning
confidence: 99%
“…Note that a modification of the model such as in Ref. 26 is not necessary here, as the spin-orbit interaction is comparatively weak in the III-nitrides, which leads to spin splittings two orders of magnitude smaller than the band gap.…”
Section: B Empirical Tight-binding Modelmentioning
confidence: 99%
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“…The interesting optical and structural properties of ZnTe/CdSe superlattices (SLs) make them promising candidates for photovoltaic devices. The type‐II band alignment between ZnTe and CdSe allows the direct spatial separation of the photo‐generated carriers (Mourad & Richters, ). By varying the SLs layer thicknesses and the number of periods, it is possible to adjust the absorption of the solar cell to match the visible spectrum (Boyer‐Richard et al ., ).…”
Section: Introductionmentioning
confidence: 99%