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URN: urn:nbn:de:swb:90-447934

Constraints on Transport Models for Galactic Cosmic Rays and their Implications for the Anomalous Positron Abundance

Kunz, Simon Michael

While supernova remnants account for most of the cosmic rays in the Galaxy, they do not produce essential amounts of antimatter. The predicted amount of positrons, which are assumed to be purely secondary produced by cosmic ray interactions, cannot explain the measurements from PAMELA and very recently from AMS-02. In this work current cosmic ray transport models are investigated and the transport related uncertainty on the expected secondary positron flux is quantified.

Zugehörige Institution(en) am KIT Institut für Experimentelle Kernphysik (IEKP)
Publikationstyp Hochschulschrift
Jahr 2014
Sprache Englisch
Identifikator KITopen-ID: 1000044793
Verlag Karlsruhe
Abschlussart Dissertation
Fakultät Fakultät für Physik (PHYSIK)
Institut Institut für Experimentelle Kernphysik (IEKP)
Prüfungsdaten 14.11.2014
Referent/Betreuer Prof. W. de Boer
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