Speaker
Todor Stanev
(Bartol Research Institute and Dept. of Phys. and Astronomy, Univ. of Delaware, USA)
Description
We discuss the the models for cosmic ray acceleration to Ultra High Energy and their possible sources. We concentrate on astrophysical models. We then discuss the propagation of these UHECR from their sources to us and different models that describe the propagation. The last topic is the production of high energy signals (gamma rays and neutrinos) during propagation and the probability for their detection.
