Relativistic Radiative Flow in a Luminous Disk with Velocity-Dependent Eddington Factor

Luminosity L>LE Component ep normal plasma vs ee pair plasma Velocity mildly relativistic β=0.26, γ=1.04 highly relativistic β=0.92, γ=2.55 ultra relativistic β=0.99, γ=10 extremely relativistic β=0.9999, γ=100 In the current theoretical studies under radiative or magnetical acceleration of astrophysical jets, it can be possible to accelerate jets up to relativistic regimes on the order of 0.9c. However, no one succeed to accelerate jets up to extremely relativistic regimes of γ=10~100.