Pulsar Electrons Detection in AMS-02 Experiment. Model Status and Discovery Potential

Bibcode
2011crpa.conf..556P
DOI
10.1142/9789814329033_0069
Pochon, J.
Bibliographical reference

Cosmic Rays for Particle and Astroparticle Physics. Edited by S Giani (CERN, Switzerland), C Leroy (University of Montreal, Canada), & P G Rancoita (INFN Milano-Bicocca, Italy) . Published by World Scientific Publishing Co. Pte. Ltd., 2011. ISBN #9789814329033, pp. 556-562

Advertised on:
6
2011
Number of authors
1
IAC number of authors
1
Citations
1
Refereed citations
1
Description
The measurements of cosmic rays electrons (e±) have begun a new era a few years ago with high precision experiments like PAMELA and Fermi-LAT. Both experiments show an excess above 10 GeV. Studying Fermi-LAT data, the total electron flux seems to be steeper than expected. While these new measurements have not closed the debate, results from AMS-02 are expected to reach the accuracy needed to determine a full description of these excesses, and hopefully give some evidence on the possible source. We will present in this paper, the AMS-02 capacity in the case of positrons produced by pulsars.
Type
Non-refereed

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