Production of π Mesons and Gamma Radiation in the Galaxy by Cosmic Rays

J. B. Pollack and G. G. Fazio
Phys. Rev. 131, 2684 – Published 15 September 1963
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Abstract

A detailed analysis is presented of the most probable sources in our galaxy of gamma radiation with energy greater than 0.2 MeV. Predictions are made of the resulting fluxes and their angular distribution in the vicinity of the earth. The results of these calculation and their implications for future gamma-ray experiments and detectors are discussed.

  • Received 15 May 1963

DOI:https://doi.org/10.1103/PhysRev.131.2684

©1963 American Physical Society

Authors & Affiliations

J. B. Pollack*

  • Astronomy Department, Harvard University, Cambridge, Massachusetts

G. G. Fazio

  • Smithsonian Astrophysical Observatory and Harvard College Observatory, Cambridge, Massachusetts

  • *National Science Foundation Predoctoral Fellow.

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Issue

Vol. 131, Iss. 6 — September 1963

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