1993
DOI: 10.1016/0022-0248(93)90657-i
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Influence of growth conditions on the photoluminescence of pseudomorphic MBE grown Si1-xGex quantum wells

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Cited by 10 publications
(4 citation statements)
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“…The consequence here is the enhancement of the PL intensity of sample C compared with sample B due to a stronger carrier confinement. Meanwhile, the PL intensities of samples D and E are weaker than that of sample C, although the experimentally and theoretically predicted band offsets at the conduction and valence band edges are larger than those of sample C. From the discussion in figure 2, this result could be attributed to the influence of point defects in the Ge 1−x Sn x layer, meaning that these defects act as non-radiative recombination centers by reducing the PL intensity [22]. Considering these results, not only large energy band offsets but also high crystallinity in double heterostructures are essential to enhance the efficiency of PL emission.…”
Section: Resultsmentioning
confidence: 87%
“…The consequence here is the enhancement of the PL intensity of sample C compared with sample B due to a stronger carrier confinement. Meanwhile, the PL intensities of samples D and E are weaker than that of sample C, although the experimentally and theoretically predicted band offsets at the conduction and valence band edges are larger than those of sample C. From the discussion in figure 2, this result could be attributed to the influence of point defects in the Ge 1−x Sn x layer, meaning that these defects act as non-radiative recombination centers by reducing the PL intensity [22]. Considering these results, not only large energy band offsets but also high crystallinity in double heterostructures are essential to enhance the efficiency of PL emission.…”
Section: Resultsmentioning
confidence: 87%
“…It is suggested that these high-density point defects play function as nonradiative recombination centers. 26) As a result, in the H-irradiated Ge 1−x Sn x layer, nonradiative recombination through point defects may be more dominant than radiative recombination with the indirect transition, while radiative recombination with the direct transition is still observable. This is because the radiative recombination with the indirect transition needs a longer recombination time of the microseconds order than that with the direct transition of the nanoseconds order.…”
Section: Resultsmentioning
confidence: 99%
“…4. Measurement data is taken from (16)(17)(18)(19). The temperature dependence of E g is modeled for each material after Varshni (20) as…”
Section: Bandgapmentioning
confidence: 99%