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See also M. Grundmann, N. N. Ledentsov, O. Stier, D. Bimberg, V. M. Ustinov, P. S. Kopev, Z. I. Alferov, 68, 979 (1996).
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Jpn. J. Appl. Phys.
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18
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22244435377
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The PL spectra at 80 K are essentially identical, except for a ∼4 meV redshift
-
The PL spectra at 80 K are essentially identical, except for a ∼4 meV redshift.
-
-
-
-
20
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22244455862
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-
These two transitions, and the QD5 transition, are unresolved in the PL spectra, even at high excitation density, and so the fifth Gaussian peak in the fits represents a convolution of their PL response
-
These two transitions, and the QD5 transition, are unresolved in the PL spectra, even at high excitation density, and so the fifth Gaussian peak in the fits represents a convolution of their PL response.
-
-
-
-
22
-
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22244449771
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The sloping background to the QD spectrum made the determination of the PR modulus unreliable here (See Ref. 4)
-
The sloping background to the QD spectrum made the determination of the PR modulus unreliable here (See Ref. 4).
-
-
-
-
23
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0005984188
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Y. T. Dai, J. C. Fan, Y. F. Chen, R. M. Lin, S. C. Lee, and H. H. Lin, J. Appl. Phys. 82, 4489 (1997).
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Lee, S.C.5
Lin, H.H.6
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24
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22244492727
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private communication
-
P. Maksym (private communication).
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Maksym, P.1
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