Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin

Details Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin

Apr 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970natur.226..135f&link_type=abstract

Nature, Volume 226, Issue 5241, pp. 135-136 (1970).

Mathematics

Logic

64

Scientific paper

RECENT work by one of us (F. W. S.) has emphasized the possible cosmological significance of the study of the isotropic component of cosmic γ-radiation between 1 and 100 MeV energy1-3. Vette et al. (ref. 4 and unpublished) have presented evidence for a new component of isotropic γ-radiation above 1 MeV energy being distinct in nature and origin from that at lower energies. At present, these data are consistent only with the hypothesis previously discussed5,6 that these γ-rays are the redshifted remnant of cosmic-ray interactions producing pions at an earlier stage in the evolution of the universe corresponding to a redshift z~=100.

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