In the cold unmagnetized linear plasma model, the refractive-index relation is n2=1−ωp2/ωL2, withThe critical density occurs at ωp=ωL=2πc/λL. Thusfor λL=1μm. The corresponding frequency isA propagating conventional laser wake generally uses an underdense plasma, rather than this cutoff density. Strong relativistic laser motion, collisions or a magnetized plasma modify this simple critical-density condition.
ωp2=ϵ0menee2.
ncrit=e2ϵ0me(λL2πc)2≃1.12×1027m−3=1.12×1021cm−3,
ωp≃1.88×1015rads−1,fp=ωp/(2π)≃3.0×1014Hz.
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