Acceleration of particles in Gamma Ray sources: Blazars and Gamma Ray Bursts

Details Acceleration of particles in Gamma Ray sources: Blazars and Gamma Ray Bursts Acceleration of particles in Gamma Ray sources: Blazars and Gamma Ray Bursts

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..289p&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 289-298 (2001).

Astronomy and Astrophysics

Astronomy

1

Active And Peculiar Galaxies And Related Systems, Unidentified Sources Of Radiation Outside The Solar System, Radiation Mechanisms, Polarization

Scientific paper

The objectives of my talk are to indicate the requirements for particle acceleration for both electrodynamic models and hadronic models in blazars, then to propose a relativistic Fermi acceleration process to achieve the goal of UHE Cosmic Ray production in relativistic flows. Relativistic magnetic fronts, when they cross each other, produce an efficient Fermi process. It is also indicate how forward and backward fronts can be generated. Most of the involved physics also apply to Gamma Ray Bursts provided that they are produced by a magnetically collimated relativistic flow. .

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