Modeling Particle Acceleration in AGN's

Details Modeling Particle Acceleration in AGN's Modeling Particle Acceleration in AGN's

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.2683l&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The radiation from Active Galactic Nuclei of the Blazar class is commonly attributed to synchrotron emission and inverse Compton scattering of a population of relativistic electrons (and positrons) accelerated inside the jets of the source. In this work we discuss the ambiguities that are present in the determination of the parameters of the model such as the size the source region, its Doppler factor, the magnetic field and the maximum electron energy in the jet frame.

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