Charged particles in the magnetosphere of a collapsing star

Details Charged particles in the magnetosphere of a collapsing star Charged particles in the magnetosphere of a collapsing star

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2....8k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 8-14. In Russian.

Physics

2

Charged Particles, Gravitational Collapse, Stellar Atmospheres, Stellar Magnetospheres, Stellar Physics, Drift Rate, Electromagnetic Fields, Particle Motion, Particle Trajectories

Scientific paper

The motion of charged particles in the external electromagnetic field of a collapsing star (CS) is examined in the drift approximation. It is shown that the energy of charged particles in the magnetosphere of a CS varies according to a power law. The rate of change of particle energy depends on particle energy, collapse phase, and the location of particles relative to the equatorial plane of the star. The relation between the rate of energy accumulation by particles and synchrotron losses also changes in the course of the collapse.

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