1991
DOI: 10.1109/3.73540
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Optical line shape functions in quantum-well and quantum-wire structures

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Cited by 52 publications
(15 citation statements)
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“…We have used here the Gaussian homogeneous lineshape function instead of the Lorentzian lineshape which results in an underestimation of the gain (Ohtoshi and Yamanishi 1991;Asada 1993). From the complex susceptibility in Eq.…”
Section: The Modelmentioning
confidence: 98%
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“…We have used here the Gaussian homogeneous lineshape function instead of the Lorentzian lineshape which results in an underestimation of the gain (Ohtoshi and Yamanishi 1991;Asada 1993). From the complex susceptibility in Eq.…”
Section: The Modelmentioning
confidence: 98%
“…It influences the dynamics of semiconductor and hence plays an important role in describing the device's performance under CW operation as well as frequency chirp under high speed modulation (Schneider et al 2004). The QD material is theoretically predicted to have small ∂(δn)/∂N at each resonant state (Schneider et al 2002) and results in α ≈ 0. This is inherent to QDs which have "atom like" properties with more confinement and a symmetric gain profile.…”
Section: Carrier Induced Materials Dispersion and αmentioning
confidence: 99%
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“…2 Theoretical approach with taking into account the non-Markovian processes can be served as substantiation of such a character of the emission line. 3,4 However, the known methods of the emission line calculations are complex and performed only numerically that makes difficulties for considering the influence of excitation conditions and parameters of semiconductor materials on the radiative recombination spectra.…”
Section: Introductionmentioning
confidence: 99%
“…In contrast to the approximation in [3], where the analysis of the spontaneous emission spectra was performed on the basis of an equation that describes interaction of one electron-hole pair with an effective medium and including the effects of broadening in a phenomenological form, in the model presented, two or three interacting electron-hole pairs are analyzed, whereas the broadening of emission lines occurs naturally due to the splitting of the energy levels of many-particle states. In the model of [3], factorization of many-particle operators in which one eliminates from consideration the non-Markovian effects that lead, as is known, to the deviation of the emission line profile from the Lorenzian one [4][5][6], is used. In direct solution of the many-particle Schro .. dinger equation, the necessity in factorization is absent, and the effects of non-Markovian dephasing of the interband polarization are taken into account implicitly.…”
mentioning
confidence: 99%