Dr Paul Kinsler. [Acknowledgements & Feedback]
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<> AU: RIDLEY_BK, ALDOSSARY_O, CONSTANTINOU_NC, BABIKER_M <> NA: UNIV ESSEX,DEPT PHYS,WIVENHOE PK,COLCHESTER CO4 <> 3SQ,ESSEX,ENGLAND <> JN: PHYSICAL REVIEW B-CONDENSED MATTER, 1994, Vol.50, No.16, <> pp.11701-11709 <> IS: 0163-1829 <> AB: Optical vibrations of a thin ionic slab are described by a <> macroscopic theory involving the hybridization of LO, TO, and <> interface-polariton modes. The resultant modes are triple <> hybrids, which satisfy both elastic and electromagnetic <> boundary conditions at the two surfaces. Analytic expressions <> are derived for the relative ionic displacements and related <> electric fields, and for the dispersion relations, assuming <> elastic isotropy and neglecting retardation effects. Comparison <> of mode patterns with those obtained by Fuchs and Kliewer, who <> used electromagnetic boundary conditions only, show that Fuchs- <> Kliewer modes are a good approximation to the system of the <> triple-hybrid modes our theory describes. <> KP: ELECTRON-PHONON INTERACTION, GAAS-ALAS SUPERLATTICES, QUANTUM- <> WELLS, DOUBLE HETEROSTRUCTURES, FROHLICH INTERACTION, <> DISPERSION, SCATTERING
LO-phonon, TO-phonon, IP_phonon
They refer to optical strains S_{alpha beta} (defined below).
However, they actually use
T_{alpha beta}, the "elastic stress" as their boundary-condition,
which they do not define
(or reference), but which is related to S_{alpha beta}.
S_{alpha beta} = - (1 / 2) ( du_{alpha} / d{beta} + du_{beta} / d{alpha} )
alpha, beta = x, y, z
p11702: s-polarized TO-phonon modes have zero electric fields everywhere. Thus no hybidisation is required for this type of mode. ... NB: p-polarised TO-phonon
p11702: LO-phonon -- IP-phonon hybrid-phonons can satisfy EM boundary-conditions (DC-model) but cannot satisfy elastic conditions nwithout neglecting shear stress. The latter approach is the one adopted by Constantinou-AR-1993 (ref 30).
XINDEX: log-file, hybrid-phonon, boundary-condition, TO-phonon, Ridley-1993, Babiker-Z-1998, index-file, log-file.
19971209 10 11
Email Feedback: Dr.Paul.Kinsler@physics.org
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