C. Prévotat, Zh. Zhu, S. Koldobskiy, A. Neronov, D. Semikoz, M. Ahlers
As cosmic rays propagate through the Galaxy, they produce gamma rays and contribute to the gamma-ray background. The authors compute the expected gamma-ray background based on the observed cosmic ray flux. They show an overproduction of gamma-ray above 100 TeV, which they suggest is due to the rarity of 1 PeV cosmic-ray sources. Their work helps constrain the sources of high energy cosmic rays.