Filamentary instability at realistic stopping power of nuclear matter

Evolution of filamentary instability in relativistic nucleus-nucleus collisions is studied within the framework of the two-fluid dynamic model with mean mesic fields. A model problem of interpretation of two infinite nuclear fluids is considered. It is shown that the deceleration and excitation of fluids are accompanied by the appearance of oscillations induced by the wave dynamics of mesic fields. It has been demonstrated that, despite the strong deceleration of nuclear fluids, the filamentary instability remains strong in this system