Use quasineutrality, ne=Zni. Multiplying the supplied collision time by the electron plasma frequency and using the preceding definition givesThus τei≫2π/ωp requires ND≫(2π/9.6)ZlnΛ; for ordinary Z and lnΛ∼1–30, this is a large plasma parameter. Many particles then collectively screen a charge, fluctuations in a Debye sphere are relatively small, and mean-field electrostatics descriptions become meaningful. A large plasma parameter is also associated with weak Coulomb coupling, well-separated screening and close-collision scales, and collective plasma oscillations surviving many oscillations before collisionally relaxing. Roughly, relative counting fluctuations scale as ND−1/2 and the ratio of interaction to thermal energy decreases as ND increases. Small ND signals that strong correlations can invalidate the simple weakly coupled plasma description.
ωpτei=ZlnΛ9.6ND.
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