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 ( \\omega _{ce}\\tau _{e} \\ll 1 ), 2) a collision-induced mode supported by the thin-layer waves when \\omega _{ce}\\tau _{e} g\\sim 1 , 3) a corresponding collision-induced mode supported by the bulk space-charge waves when \\omega _{ce}\\tau _{e} g\\sim 1 , 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
Link To Document :
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