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Ultrahigh Energy Gamma-raysAn analysis is made of the interactions of very high energy cosmic ray protons with the relict radiation in extragalactic space. Two situations are examined: gamma rays derived from neutral pions -mesons produced in collisions in a nonevolutionary situation and gamma rays from electron pairs produced at early epochs. It is shown that the ultrahigh energy gamma rays could conceivably be of high enough intensity to be detected. The flux of gamma rays from the second process is not far from the diffuse background that was reported.
Document ID
19730020034
Document Type
Conference Paper
Authors
Strong, A. W.
(Durham Univ.)
Wdowczyk, J.
(Durham Univ.)
Wolfendale, A. W.
(Durham Univ.)
Date Acquired
August 7, 2013
Publication Date
June 1, 1973
Publication Information
Publication: NASA. Goddard Space Flight Center Intern. Symp. and Workshop on Gamma-Ray Astrophysics
Subject Category
Space Radiation
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19730020021Analytic PrimaryInternational symposium and workshop on gamma-ray astrophysics
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