pith. sign in

In the above expressions, the Bickley functionKi n(z) appears defined as [51] Ki n (z)≡ Z ∞ 0 e−zcoshx 1 coshn x dx.(39) Below, the dependence onzofKi n(z) will be suppressed

A32 = κ(−2ω+iγ)K 3/2 2 γ2 p −z3K 3 1 −7z 2K 2 1 K2 +z(−9 +z 2)K1K 2 2 + 4(3 +z 2)K 3 1 , A33 = Ki 1κ2z3 −z(κ 2(3 +z 2) + 5ω(ω−iγ))K 1 + (κ2(−12 +z 2)−20ω(ω−iγ))K 2 5γ2(zK1 + 4K2)

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Normal mode analysis within relativistic massive transport

hep-ph · 2025-05-07 · unverdicted · novelty 7.0

Normal mode analysis of the relativistic Boltzmann equation for massive particles reveals coupling between sound and heat channels, mass-dependent critical wavenumbers, and an infinite branch cut for Landau damping.

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  • Normal mode analysis within relativistic massive transport hep-ph · 2025-05-07 · unverdicted · none · ref 3

    Normal mode analysis of the relativistic Boltzmann equation for massive particles reveals coupling between sound and heat channels, mass-dependent critical wavenumbers, and an infinite branch cut for Landau damping.