Tracing high-energy interactions in the Universe with neutrinos
by
On-line only
CERN
Abstract:
The existence of astrophysical neutrinos has been firmly established in the past decade. Possible connections of high-energy neutrinos with astrophysical sources have been found by IceCube, and theory studies have been improving in explaining these connections. The recent measurement by Km3Net reporting about an exceptionally high-energy event has contributed to the excitement in the field, and pushed several speculations about its possible origin.
In this seminar I will present some of the recent experimental findings on high-energy neutrinos, as well as models for the interpretation of these results, with a multimessenger view. I will discuss how cosmogenic neutrinos could help in deciphering the redshift distribution of astrophysical sources of high-energy particles, as well as the fraction of protons in the ultra-high-energy cosmic rays. In addition, I will report about how source modelling advances our understanding of the possible associated sources, as well as the region of the source where neutrinos could be originated.
Carmelo Evoli, Sébastien Renaux-Petel, Alessandra Silvestri