Hydrodynamic description of neutrino gas

The system of neutrino-antineutrino (νν̄) plasma is considered taking into account their weak Fermi interaction. New fluid instabilities driven by strong neutrino flux in a plasma are found. The nonlinear stationary as well as nonstationary waves in the neutrino gas are discussed. It is shown that a bunch of neutrinos, drifting with a constant velocity across a homogeneous plasma, can also induce emission of lower energy neutrinos due to scattering, i.e. the decay of a heavy neutrino νH into a heavy and a light neutrino νL (νH → νHνL) in a plasma. Furthermore we find that the neutrino production in stars does not lead in general to energy losses from the neutron stars.