Very high energy photons and neutrinos: Implications for UHECR
Bartol Research Institute and Dept. of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA
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Depending on the environment of the acceleration processes for ultra-high energy cosmic rays, photons and neutrinos may be produced by interactions in the sources. If so, observations of gamma-rays or neutrinos could pinpoint the sources. This paper reviews some aspects of the search for photons and neutrinos from possible sources of ultra-high energy cosmic rays.
© Owned by the authors, published by EDP Sciences, 2013
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