Relativistic jets and non-thermal radiation from collapse of stars to black holes

Details Relativistic jets and non-thermal radiation from collapse of stars to black holes Relativistic jets and non-thermal radiation from collapse of stars to black holes

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..238..395k&link_type=abstract

Black Holes from Stars to Galaxies -- Across the Range of Masses. Edited by V. Karas and G. Matt. Proceedings of IAU Symposium #

Physics

Scientific paper

The formations of relativistic jets in the stars magnetospheres on the stage of the stellar gravitational collapse to black holes are considered. These jets will formed in the polar caps of collapsing stars magnetospheres, when the stellar magnetic field increases during collapse and the charged particles will be accelerate. These jets will generate the non-thermal radiation. The analysis of particle dynamics and its emission in the stellar magnetosphere under collapse show that the stars on the stage of gravitational collapse must by powerful sources of the relativistic jets and the non-thermal radiation. The radiation flux grows with decreasing stellar radius and can be observed in the form of radiation burst in wide band wave- from radio to gamma-ray. These bursts radiation can be observed as gamma- and X- rays bursts.

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