Probing extreme astrophysical accelerators through neutrino anisotropy

Abstract

We present the extent to which anisotropies in the ultrahigh energy neutrino sky can probe the distribution of extreme astrophysical accelerators in the universe. In this talk, we discuss the origin of an anisotropic neutrino sky and show how observers can use this anisotropy to measure the evolution of ultrahigh energy neutrino sources - and therefore, the sources of ultrahigh energy cosmic rays - for the very first time.

References in corpus (7)

• Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above $8\times 10^{18}$ eV
• The Laniakea supercluster of galaxies
• Characteristics of the diffuse astrophysical electron and tau neutrino flux with six years of IceCube high energy cascade data
• Wiener Reconstruction of Large-Scale Structure from Peculiar Velocities
• The optical depth of the Universe to ultrahigh energy cosmic ray scattering in the magnetized large scale structure
• The Imprint of Large Scale Structure on the Ultra-High-Energy Cosmic Ray Sky
• Cosmic-Ray Anisotropy from Large Scale Structure and the effect of magnetic horizons