Linear stability analysis of relativistic magnetized jets - The Kelvin-Helmholtz mode

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Table 1.

Parameters for the fiducial cases examined.

Case	ρ₀	η	γ	σ	ϖ₀	ω
F	1	10	2	1	0.1	1.34+0.68i
F5	1	10	5	1	0.1	2.44+0.31i

Notes. The unit for density is arbitrary. The values of ω correspond to k = π. We reiterate that η = ρ_e/ρ₀, where ρ_e is the density of the environment. The magnetization is defined in Eq. (4), and ϖ₀ controls the distribution of the magnetic field given by Eqs. (2) and (3).

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