| Popis: |
We consider how the cutoff of the ultrahigh energy neutrino spectrum introduces an effective neutrino horizon, allowing for future neutrino detectors to measure an anisotropy in neutrino arrival directions driven by the local large-scale structure. We show that measurement of the level of this anisotropy along with features of the neutrino spectrum will allow for a measurement of the evolution of ultrahigh energy neutrino sources, which are expected to also be the sources of ultrahigh energy cosmic rays. |
