2003
DOI: 10.1103/physrevb.68.035316
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Interplay of phonon and disorder scattering in semiconductor quantum wells

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Cited by 14 publications
(7 citation statements)
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“…To allow for easier comparison of the spectral shape, the energy scale is chosen relative to the 1s-exciton absorption peak at 1.4650 eV (70 K), 1.4681 eV (50 K), and 1.4697 eV (30 K). The line broadens only slightly in this temperature range 23 . The corresponding PL spectra are shown on a linear scale (middle) and on a semi-logarithmic scale (right).…”
Section: A Correlated Plasma Regimementioning
confidence: 76%
“…To allow for easier comparison of the spectral shape, the energy scale is chosen relative to the 1s-exciton absorption peak at 1.4650 eV (70 K), 1.4681 eV (50 K), and 1.4697 eV (30 K). The line broadens only slightly in this temperature range 23 . The corresponding PL spectra are shown on a linear scale (middle) and on a semi-logarithmic scale (right).…”
Section: A Correlated Plasma Regimementioning
confidence: 76%
“…It is expected that at very low temperatures, where the exciton-phonon scattering is not very efficient, the exciton PL spectra are mostly inhomogeneously broadened and have Gaussian convolution, while the line shape becomes more like a Lorentzian at higher temperatures. The exciton-acoustic-phonon interaction coefficient used are a ≈ 2−10 µeV/K [14][15][16][17] and the exciton-LO-phonon interaction coefficient is taken to be b ≈ 10−15 meV [15][16][17][18]. Values obtained for our samples are the following: Γ 0 ≈ 2 meV, Γ (T = 77 K) ≈ 3 meV, Γ (T = 300 K) ≈ 9 meV, which agrees well with the results of the above-mentioned authors and theoretical predictions.…”
Section: Photoluminescence Spectra and Discussionmentioning
confidence: 99%
“…The Einstein A coefficient, or spontaneous emission rate, is [32] γ sp = 9n where γ spo is the spontaneous emission rate in the vacuum, n and n QD are the refractive index of the medium and the QD, respectively. By inserting the parameters into Eq.…”
mentioning
confidence: 99%