Abstract
Understanding cosmic acceleration mechanisms, such as jet formation in black holes, star collapses or binary mergers, and the propagation of accelerated particles in the universe is still a ’work in progress’ and requires a multi-messenger approach, exploiting the complementarities across all possible probes: ultra-high energy cosmic rays (UHECR), gammarays and neutrinos. In this report the IceCube results concerning searches for astrophysical neutrino point sources and diffuse fluxes from populations of sources widely distributed in the sky or from the GZK cut-off will be summarized. The results to other Neutrino Telescopes and to astrophysical models of neutrino production in sources will be compared.
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