Gamma-Ray Echo as a Probe of Supernova Neutrino Emission Anisotropy and Long-Baseline Effects
This paper proposes that comparing the electron antineutrino flux inferred from a core-collapse supernova's gamma-ray echo with that detected on Earth can serve as a powerful probe for testing large neutrino emission anisotropies and long-baseline propagation effects, thereby motivating the development of next-generation MeV gamma-ray telescopes.