Diffuse gamma radiation at ultrahigh energies of greater than about 10 to the 14th eV

Details Diffuse gamma radiation at ultrahigh energies of greater than about 10 to the 14th eV Diffuse gamma radiation at ultrahigh energies of greater than about 10 to the 14th eV

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..873b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Oct. 1988, p. 873-881. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Diffuse Radiation, Energetic Particles, Galactic Cosmic Rays, Galactic Radiation, Gamma Ray Astronomy, High Energy Interactions, Isotropic Media, Milky Way Galaxy, Point Sources

Scientific paper

Diffuse fluxes of ultrahigh-energy gamma radiation were calculated from cosmic rays in the Galactic disk, cosmic rays in the intergalactic medium interacting with microwave background radiation, and point extragalactic sources. A considerable flux of isotropic gamma radiation is produced due to the interaction of ultrahigh-energy cosmic rays with the microwave background radiation if cosmic rays observed at E greater than about 10 to the 18th eV are metagalactic photons. This flux can be detected in the direction perpendicular to the Galactic plane.

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