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Search for Cosmic-Ray Antiparticles with Balloon-borne and Space-borne Experiments

2009/03/11 by Ph. von Doetinchem, von Doetinchem, Ph.
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Particle Detector Development and Performance #Scientific Research and Discoveries

paper · pdf · doi:10.48550/arxiv.0903.1987

openalex publication_date 2009/03/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

This thesis discusses two different approaches for the measurement of cosmic-ray antiparticles in the GeV to TeV energy range. The first part of this thesis discusses the prospects of antiparticle flux measurements with the proposed PEBS detector. The project allots long duration balloon flights at one of Earth's poles at an altitude of 40 km. GEANT4 simulations were carried out which determine the atmospheric background and attenuation especially for antiparticles. The second part covers the AMS-02 experiment which will be installed in 2010 on the International Space Station at an altitude of about 400 km for about three years to measure cosmic rays without the influence of Earth's atmosphere. The present work focuses on the anticoincidence counter system (ACC). The ACC is needed to reduce the trigger rate during periods of high fluxes and to reject external particles crossing the tracker from the side or particles resulting from interactions within the detector which would otherwise disturb the clean charge and momentum measurements. The last point is especially important for the measurement of antinuclei and antiparticles.

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