• 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