Use collisional inverse bremsstrahlung in a weakly coupled, unmagnetized plasma. The specified density is ne=1026m−3, and kBT=1000eV. The electron Debye length is 2.35×10−8m, the plasma frequency is 5.64×1014s−1, and the laser angular frequency is ω=2πc/λ=1.79×1015s−1. Thus X=ωp2/ω2≃0.099<1: the plasma is underdense and a propagating wave exists.
Estimate bmin as the larger of the classical Coulomb-deflection length Ze2/(4πϵ0kBT) and the electron quantum length ℏ/mekBT. Both are about 9×10−12m here, giving lnΛC≃8. With the usual thermal collision convention,The Z factor follows from niZ2=neZ.[ref]
νei≃2.91×10−6Te[eV]3/2ne[cm−3]ZlnΛCs−1≃4.4×1011s−1.
NRL Plasma Formulary (2019). Coulomb collision-rate normalization and thermal parameters; densities in cubic centimetres and temperatures in eV
The weakly collisional Drude model gives ϵr=1−ωp2/[ω(ω+iνei)] for fields proportional to e−iωt. Expanding at νei≪ω yields a real refractive index nr=1−X≃0.949 and intensity attenuation coefficientConsequently the intensity e-folding absorption length isi.e. of order a centimetre. Taking a Coulomb logarithm between about 5 and 10 gives roughly 5–10mm. The electric-field amplitude decay length is twice this intensity length. This estimate assumes a uniform slab thick enough to define an absorption length and neglects gradients, nonlinear quiver heating and other absorption mechanisms.
αI=2Imk≃cνei1−XX.
LI=νeiXc1−X≃6.6×10−3m,
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