1993
DOI: 10.1103/physrevlett.71.3717
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Direct measurement of heavy-hole exciton transport in type-II GaAs/AlAs superlattices

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Cited by 34 publications
(20 citation statements)
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“…19͑b͔͒ starts to decrease at even higher excitation intensities of about 100 W/cm 2 , indicating that the mobility is high enough to reach the sparsely distributed nonradiative recombination sites. 65 This implies that the QB PL is saturated, in agreement with the experimental data ͓dots in Fig. 19b͔.…”
Section: Samples With Strong Type-ii Charactersupporting
confidence: 80%
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“…19͑b͔͒ starts to decrease at even higher excitation intensities of about 100 W/cm 2 , indicating that the mobility is high enough to reach the sparsely distributed nonradiative recombination sites. 65 This implies that the QB PL is saturated, in agreement with the experimental data ͓dots in Fig. 19b͔.…”
Section: Samples With Strong Type-ii Charactersupporting
confidence: 80%
“…Thus the decay of the QB PL is mainly controlled by the decay of the (X z 1-hh1͒ exciton density via the QB's and nonradiative traps. 65 A similar case evolves at higher excitation densities ͓Figs. 18͑e͒ and ͑f͔͒ of about 1ϫ10 12 /cm 2 .…”
Section: Samples With Strong Type-ii Charactermentioning
confidence: 88%
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“…These decay characteristics are explained by our recently proposed defect-trapping model. 10,14 At low temperatures, the excitons are in localized states and decay radiatively. At higher temperatures, the excitons begin to populate mobile states, and they may diffuse along the interface until they interact with defects which cause them to decay nonradiatively.…”
Section: Resultsmentioning
confidence: 99%
“…The mixing of the X z and ⌫ subbands due to the superlattice structure in the ͓001͔ growth direction was investigated both experimentally [5][6][7] and theoretically. 8,9 The interface roughness of the structures plays an important role for the indirect exciton mobility [10][11][12][13][14] and for the mixing of the X x,y subbands with the ⌫ subband in the ͓001͔ growth direction 12 and all X subbands for growth directions other than ͗100͘.…”
Section: Introductionmentioning
confidence: 99%