Computer Science
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..421k&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 421-424
Computer Science
Scientific paper
The particles acceleration and its non-thermal emission in the magnetospheres of collapsing stars are considered. The magnetic field in magnetosphere increases considerably, when the star is compressed under the collapse. The charged particles will be accelerated in this field. These particles will generate radiation when moving in the magnetic field. The effect can be observed by means of modern instruments [7]. The radiation flux grows during a stellar collapse in millions times and can be observed in the form of radiation pulse with duration equal to the stellar collapse time. This flux depends on the distance to the star, its magnetic field, and the particle spectrum in the magnetosphere. In this paper the radiation fluxes are calculated for various collapsing stars with the initial dipole magnetic fields and the initial power-series, relativistic Maxwell, and Boltzmann particles energy distributions in the magnetosphere.
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