The applicability of the infinite-barrier scheme to the study of the confinement mechanism for the optical phonons in GaAs/AlxGa1-xAs heterostructures is critically addressed. In the framework of a bond-charge-model calculation, we demonstrate that the line shape of LO1 GaAs-like displacement patterns differs from a sinelike function and depends on the Al content of the ternary barrier, preventing the extension of the infinite-barrier scheme to ternary systems. Finally, the analysis of Raman intensities is indicated as a suitable probe of the confinement efficiency because of its sensitivity to the displacement pattern line shape. © 1994 The American Physical Society.

Molteni, C., Colombo, L., Miglio, L., Benedek, G. (1994). Barrier height versus confinement efficiency for the optical phonons in GaAs/AlxGa1-xAs heterostructures. PHYSICAL REVIEW. B, CONDENSED MATTER, 50(16), 11684-11686 [10.1103/PhysRevB.50.11684].

Barrier height versus confinement efficiency for the optical phonons in GaAs/AlxGa1-xAs heterostructures

MIGLIO, LEONIDA;BENEDEK, GIORGIO
1994

Abstract

The applicability of the infinite-barrier scheme to the study of the confinement mechanism for the optical phonons in GaAs/AlxGa1-xAs heterostructures is critically addressed. In the framework of a bond-charge-model calculation, we demonstrate that the line shape of LO1 GaAs-like displacement patterns differs from a sinelike function and depends on the Al content of the ternary barrier, preventing the extension of the infinite-barrier scheme to ternary systems. Finally, the analysis of Raman intensities is indicated as a suitable probe of the confinement efficiency because of its sensitivity to the displacement pattern line shape. © 1994 The American Physical Society.
Articolo in rivista - Articolo scientifico
Phonons
English
1994
50
16
11684
11686
none
Molteni, C., Colombo, L., Miglio, L., Benedek, G. (1994). Barrier height versus confinement efficiency for the optical phonons in GaAs/AlxGa1-xAs heterostructures. PHYSICAL REVIEW. B, CONDENSED MATTER, 50(16), 11684-11686 [10.1103/PhysRevB.50.11684].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/44081
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