Origin of Cosmic Electrons from About 102 to 106 GeV

Details Origin of Cosmic Electrons from About 102 to 106 GeV Origin of Cosmic Electrons from About 102 to 106 GeV

Nov 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..27.1309r&link_type=abstract

Physical Review Letters, vol. 27, Issue 19, pp. 1309-1312

Physics

9

Scientific paper

The origin of high-energy cosmic electrons is considered. It is found that electrons of energies <~103 GeV could have been produced by local supernovae associated with known radio remnants. At higher energies, observations of muon-poor air showers indicate the existence of electrons at 106 GeV which may have originated entirely from the supernova Vela X.

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