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Cosmology with 100-TeV γ-ray telescopes

F. Halzen

R. J. Protheroe

T. Stanev and H. P. Vankov*

  • Department of Physics, University of Wisconsin, Madison, Wisconsin 53706

  • Department of Physics and Mathematical Physics, University of Adelaide, Adelaide, South Australia 5001, Australia

  • Bartol Research Institute, University of Delaware, Newark, Delaware 19716

  • *On leave of absence from the Institute for Nuclear Research and Nuclear Energy, Sofia 1784, Bulgaria.

Phys. Rev. D 41, 342 – Published 15 January, 1990

DOI: https://doi.org/10.1103/PhysRevD.41.342

Abstract

We show that the secondary photons which are by-products of the energy loss of extragalactic cosmic rays interacting with the cosmic background have a characteristic energy of 10-100 TeV. For a model where the extragalactic cosmic rays are uniformly distributed in space and in time over the past 109 yr the flux of 100-TeV photons is 105 of the cosmic-ray flux. Such fluxes are attractively close to the resolution of the new generation of γ-ray telescopes and their detection can provide important cosmological information.

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