High energy cosmic rays from active galactic nuclei

Details High energy cosmic rays from active galactic nuclei High energy cosmic rays from active galactic nuclei

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..69.2885p&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 69, no. 20, p. 2885-2888.

Astronomy and Astrophysics

Astronomy

63

Active Galactic Nuclei, Energetic Particles, Galactic Cosmic Rays, Particle Acceleration, Black Holes (Astronomy), Flux Density, Radiation Distribution

Scientific paper

Stecker et al. (1991) recently showed that if particle acceleration occurs in the central regions of AGN, then a diffuse flux of high energy neutrinos from unresolved AGN may be observable with proposed neutrino telescopes. Here, the consequences of this scenario for the production of high energy cosmic rays are examined. It is suggested that at an energy of 10 exp 16 eV, and possibly even up to 10 exp 19 eV, a substantial fraction of the observed cosmic rays may originate in the central regions of AGN.

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