A rotating magnetized plasma model with cosmic-ray pressure and diffusion yields modified dispersion, Korteweg-de Vries-Burgers, and nonlinear Schrödinger equations, with cosmic rays reducing modulation-instability growth.
The coefficients M and N are modified due to the inclusion of cosmic ray pressure, which affects the growth of the instability
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Dynamics and modulation of cosmic ray modified magnetosonic waves in a galactic gaseous rotating plasma
A rotating magnetized plasma model with cosmic-ray pressure and diffusion yields modified dispersion, Korteweg-de Vries-Burgers, and nonlinear Schrödinger equations, with cosmic rays reducing modulation-instability growth.