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2012

B/C ratio and the PAMELA positron excess

Kachelriess, M., Ostapchenko, S.

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We calculate the diffuse intensity of cosmic ray (CR) nuclei and their secondaries in the Boron-Carbon group produced by supernova remnants (SNR).

The trajectories of charged particles in the SNR are modeled as a random walk in the test particle approximation.
Secondary production by CRs colliding with gas in the SNR is included as a Monte Carlo process, while we use Galprop to account for the propagation and interactions of CRs in the Galaxy.
In the vicinity of a source, we find an approximately constant B/C ratio as a function of energy.

B/C ratio and the PAMELA positron excess · Around

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