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Fig. 1.

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Numerical solutions from linear theory and QL approach: Growth rates ( γ $ \tilde{\gamma} $) of the RH-PB instability (top) and the corresponding time evolutions for the wave energy density (second row), beam velocity (third row), and the beam temperature anisotropy (bottom) for different initial conditions: vb/vAc = 3.0, 2.5, 2.0 (left column), nb/np = 0.06, 0.03, 0.01 (second column), βc = 1.0, 0.41, 0.1 (third column), and Ab = 2.0, 1.0, 0.62 (right column). The red dots and dashed and dotted lines are explained in the text.

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