DocumentCode
1037986
Title
Electron—Hole plasma instabilities
Author
Robinson, Bruce B.
Author_Institution
RCA Laboratories, Princeton, N.J.
Volume
17
Issue
3
fYear
1970
fDate
3/1/1970 12:00:00 AM
Firstpage
200
Lastpage
206
Abstract
A semiconductor plasma slab will support three classes of slow quasi-static waves: 1) bulk waves which involve space-charge disturbance throughout the bulk of a thick slab, 2) surface waves which involve surface charge disturbance along one surface of a thick slab, and 3) thin-layer waves which involve dipolar surface charge disturbance on either side of a thin plasma slab. A review of the linear stability theory for these waves indicates that each wave class can support one or more potentially unstable two-stream modes. Four of these modes should be observable in InSb: 1) a thin-layer wave interaction in the low magnetic field limit (
), 2) a collision-induced mode supported by the thin-layer waves when
, 3) a corresponding collision-induced mode supported by the bulk space-charge waves when
, and 4) a mode which results from the interaction of surface waves. The second mode has been well documented experimentally.
), 2) a collision-induced mode supported by the thin-layer waves when
, 3) a corresponding collision-induced mode supported by the bulk space-charge waves when
, and 4) a mode which results from the interaction of surface waves. The second mode has been well documented experimentally.Keywords
Charge carrier processes; Conductors; Electrons; Frequency synchronization; Magnetic fields; Plasma stability; Plasma waves; Resonance; Slabs; Surface waves;
fLanguage
English
Journal_Title
Electron Devices, IEEE Transactions on
Publisher
ieee
ISSN
0018-9383
Type
jour
DOI
10.1109/T-ED.1970.16954
Filename
1476138
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