Origin of the High Energy Extragalactic Diffuse Gamma Ray Background

Arnon Dar and Nir J. Shaviv
Phys. Rev. Lett. 75, 3052 – Published 23 October 1995
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Abstract

Recent x-ray observations have discovered that groups and clusters of galaxies contain many more baryons in intergalactic gas than in stars. If high-energy cosmic rays are present there with an average intensity comparable to that observed in our Galaxy, they could produce the extragalactic diffuse gamma radiation.

  • Received 26 January 1995

DOI:https://doi.org/10.1103/PhysRevLett.75.3052

©1995 American Physical Society

Authors & Affiliations

Arnon Dar and Nir J. Shaviv

  • Department of Physics and Space Research Institute, Technion-Israel Institute of Technology, Haifa 32000, Israel

Comments & Replies

Dar and Shaviv Reply:

Arnon Dar and Nir J. Shaviv
Phys. Rev. Lett. 76, 3879 (1996)

Comment on the Origin of the High Energy Diffuse γ-Ray Background

F. W. Stecker and M. H. Salamon
Phys. Rev. Lett. 76, 3878 (1996)

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Vol. 75, Iss. 17 — 23 October 1995

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