Electromagnetic radiation in the collapse of stars with the relativistic Maxwell and Boltzmann particle distributions in their magnetosphere

Details Electromagnetic radiation in the collapse of stars with the relativistic Maxwell and Boltzmann particle distributions in their magnetosphere Electromagnetic radiation in the collapse of stars with the relativistic Maxwell and Boltzmann particle distributions in their magnetosphere

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..233k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 3, p. 233-239

Physics

Scientific paper

In our previous paper we considered the particles spectrum evolution and calculated the radiation flux during the collapse of the stars with initial dipole magnetic fields and an initial exponential energy distribution of particles in their magnetospheres. The calculations show that in this case the collapsing stars can be powerful sources of non-thermal radiation which can be observed by means of modern radio, X and gamma telescopes. In this paper the non-thermal radiation during the collapse of the stars with the relativistic Maxwell and Boltzmann particle distributions in the magnetospheres is investigated. The calculations were made for the stars with the gas temperature in the range 1 ev ≤ kT ≤ 10 ev. The results allow us to state that a powerful flux of non-thermal radiation which exceeds the initial flux in several billion times arises in this case.

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