Scientific Publications

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Abstract

The Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA)
has now provided a very accurate measurement of the spectrum of cosmic-ray electrons and
positrons. These results are consistent with a single power-law, but visually they suggest an
excess emission from about 100 GeV to 1 TeV, which leads to the emergence of a debate about
the existence and the source of this excess: Could come from nearby pulsars or dark-matter
annihilation? We do not know, each one has its reasons. In this work we will try to study
this controversy by clarifying this spectrum using the GALPROP code.


BibTex

@inproceedings{uniusa5370,
    title={The spectrum of cosmic ray electrons and positrons measured by the Pamela experiment: a real problem still seeking a solution},
    author={SEDRATI Rafik and Attallah reda},
    year={2013},
    booktitle={48th Rencontres de Moriond on Very High Energy Phenomena in the Universe ( March 9-16, 2013)}
}