Acceleration of the Cosmic Rays by Stellar Collapse

Physics

Scientific paper

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Scientific paper

The cosmic-rays acceleration in the magnetospheres of collapsing stars with initial dip ole magnetic fields and a certain initial energy distribution of charged particles in a magnetosphere (power-series, relativistic Maxwell, and Boltzmann distributions) are considered . When the star magnetosphere compressing under the collapse its magnetic field considerably increases. The cyclic electric field thus produced involving acceleration of charged particles. The analysis of particles dynamics and its acceleration in the stellar magnetosphere under collapse show that the collapsing stars can by powerful sources of cosmic rays and non-thermal radiation.

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