Dr Paul Kinsler. [Acknowledgements & Feedback]
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<> JN: SEMICONDUCTOR SCIENCE AND TECHNOLOGY, 1992, Vol.7, No.3B, pp.B 52-B <> 59 <> IS: 0268-1242 <> AB: Theoretical models that treat optical lattice vibrations in <> heterostructures by viewing the lattice-matched crystalline media as <> isotropic homogeneous continua separated by smooth planar interfaces, <> offer conceptual simplicity and are, without doubt, computationally <> advantageous when calculations involving electron-phonon interactions <> are carried out. The two (apparently conflicting) continuum models, <> namely the hydrodynamic (HD) and the electromagnetic (EM) models, are <> discussed, their calculational frameworks in the context of <> semiconductor heterostructures examined and some of their predictions <> displayed. A statement of the HD model in terms of a polariton subset <> plus an LO subset is given, and this permits a transparent comparison <> with the EM model to be made. It is then shown that the EM model is a <> non-dispersive, non-retarded and subsequently mishandled version of <> the polariton subset of the HD model and it completely disallows <> proper considerations of longitudinal optical modes. The sources of <> the current controversies concerning HD versus EM boundary <> conditions-confined mode identification, existence of localized alloy <> interface LO modes and interface FK modes, Frohlich-type coupling e- <> PHI together with the e-phi versus - (e/m*c)A(T).p couplings to <> electrons-are all pointed out and discussed. A close agreement <> between some very recent predictions of the two models concerning <> interface mode contributions to energy relaxation is explained and <> this helps to clarify the nature of the conflict regarding other <> contributions. Further evidence in support of the HD model from <> recent theoretical and experimental results is pointed out.
Longitudinal solutions are LO-phonons; transverse solutions are TO-phonons and IP-phonons -- these are phonon-polaritons.
XINDEX: phonon-polariton, boundary-condition, TO-phonon, LO-phonon, IP-phonon, HD-model, DC-model, index-file, log-file.
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Email Feedback: Dr.Paul.Kinsler@physics.org
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