Probing the CR positron/electron ratio at few hundreds GeV through Moon shadow observation with the MAGIC telescopes

Colin, P.; Borla Tridon, Daniela; Diago Ortega, Alicia; Doert, Marlene; Doro, M.; Pochon, Jonathan; Strah, N.; Surić, Tihomir; Teshima, M.

doi:10.48550/arxiv.1110.0183

Public

Probing the CR positron/electron ratio at few hundreds GeV through Moon shadow observation with the MAGIC telescopes

Published • Oct 2, 2011

Authors:

P. Colin

Daniela Borla Tridon

Alicia Diago Ortega

Abstract

The antimatter components measured in the Cosmic Ray (CR) flux are thought as secondary particles induced by the propagation of galactic CRs within the galaxy. Recent results from the PAMELA experiment show an unexpected increase of the positron electron ratio above 10 GeV. There could be different ...

Subject

Physics

Positron

Cosmic ray

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