Vasily S. Beskin
Published 2016-10-11Version 1
Surprisingly, the chronology of nearly 50 years of the pulsar magnetosphere and pulsar wind research is quite similar to the history of our civilization. Using this analogy, I have tried to outline the main results obtained in this field. In addition to my talk, the possibility of particle acceleration due to different processes in the pulsar magnetosphere is discussed in more detail.
Comments: 10 pages, 6 (black and white) figures, in Proceedings of the 2016 Heidelberg Symposium on High Energy Gamma-Ray Astronomy
Hybrid Simulations of Particle Acceleration at Shocks
Evidence that particle acceleration in hotspots of FR II galaxies is not constrained by synchrotron cooling
Main results of the TUS experiment on board the Lomonosov satellite
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