Large Scale Anisotropy of Cosmic Rays and Directional Neutrino Signals from Galactic Sources

Abstract

We investigate the neutrino - cosmic ray connection for sources in the Galaxy in terms of two observables: the shape of the energy spectrum and the distribution of arrival directions. We also study the associated gamma ray emission from these sources.

Proceedings of the 2nd Cosmic Ray Anisotropy Workshop, 26-28 September 2013, Madison, Wisconsin. To appear in IOP Conference Series

References in corpus (6)

• Evolution of the cosmic ray anisotropy above 10^{14} eV
• A Galactic Halo Origin of the Neutrinos Detected by IceCube
• Large scale distribution of arrival directions of cosmic rays detected above $10^{18}$ eV at the Pierre Auger Observatory
• Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory
• Cosmic Rays around $10^{18}$eV: Implications of Contemporary Measurements on the Origin of the Ankle Feature
• Outstanding Problems in Particle Astrophysics

Cited by in corpus (1)

• Estimating the contribution of Galactic sources to the diffuse neutrino flux