Abstract
The Weyl equation has been used to study the interaction of a neutrino flux with a plasma in a stellar medium. The resulting collective stimulated scattering of the neutrino by the plasma is described by a cubic dispersion relation, which is solved numerically and analytically which gives a maximum growth rate structurally identical to growth rate obtained by Bingham et al. [Phys. Lett. A 193 (1994) 279] by using a Klein–Gordon like equation model, in which the neutrinos are considered as bosons, to describe the linear regime of the collective interaction.
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