1997
DOI: 10.1007/bf02675148
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Gain and luminescence spectra of broadband emitters based on asymmetric quantum-well heterostructures

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Cited by 11 publications
(6 citation statements)
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“…The tuning range is determined by the width of the gain spectrum and hence it is rather narrow in these cases. Widening the gain spectrum is possible due to a novel conception of asymmetric quantum-well heterostructures where the potential profile in barrier regions and arrangement of differ active layers relative to current emitters play an essential role [9,10].…”
Section: Introductionmentioning
confidence: 99%
“…The tuning range is determined by the width of the gain spectrum and hence it is rather narrow in these cases. Widening the gain spectrum is possible due to a novel conception of asymmetric quantum-well heterostructures where the potential profile in barrier regions and arrangement of differ active layers relative to current emitters play an essential role [9,10].…”
Section: Introductionmentioning
confidence: 99%
“…Joining the functions at zero [C À F 1 (0) C F 2 (0)] and taking into account the normalisation condition (C À C 2), we can determine the C À and C coefécients. A combined model of the emission line broadening, in which, at the same broadening parameters, the proéle is described by a Lorentzian at DE`0 and by a Gaussian at DE b 0, was proposed in [6].…”
Section: Emission Line Broadening Proélesmentioning
confidence: 99%
“…Laser radiation is known to be the combination of spontaneous and stimulated radiations. The intensity of spontaneous radiation is specified by the velocity of spontaneous transitions [6,7]:…”
Section: Theorymentioning
confidence: 99%
“…where A cv is Einstein coefficient, d is the width of the quantum well, m rit = m c m vit /(m c + m vit ) is the reduced mass associated with the respective transversal components of the heavy or light holes (i = h, l), parameter α γ ni characterizes polarization dependence of the probability of the optical transitions and depends on the type of modes (TE or TM), levels involved (heavy or light holes), and transition energy E cv = E cni −E vni [6]; f e (E cni ) and f h (E vni ) are Fermi-Dirac distribution functions of the electrons and holes of the states E cni and E vni participating in the optical transitions [8]:…”
Section: Theorymentioning
confidence: 99%