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- W1520689607 abstract "Real breakthrough during last 1-1.5 years in cosmic ray electrons: ATIC, HESS, Pamela, and finally Fermi-LAT. New quality data have made it possible to start quantitative modeling. With the new data more puzzles than before on CR electrons origin. Need multi-messenger campaign: electrons, positrons, gammas, X-ray, radio, neutrino... It is viable that we are dealing with at least two distinct mechanisms of primary electron (both signs) production: a softer spectrum of negative electrons, and a harder spectrum of both e(+)+e(-). Exotic (e.g. DM) origin is not ruled out. Upper limits on CR electrons anisotropy are set. Good perspectives to have the Fermi LAT results on proton spectrum and positron fraction." @default.
- W1520689607 created "2016-06-24" @default.
- W1520689607 creator A5034178430 @default.
- W1520689607 date "2013-06-27" @default.
- W1520689607 modified "2023-09-27" @default.
- W1520689607 title "Fermi Lat Results and Perspectives in Measurements of High Energy Galactic Cosmic Rays" @default.
- W1520689607 hasPublicationYear "2013" @default.
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