arXiv Analytics

Sign in

arXiv:1703.05772 [astro-ph.HE]AbstractReferencesReviewsResources

Newly-Discovered Anomalies in Galactic Cosmic Rays: Time for Exotic Scenarios?

Mikhail Malkov

Published 2017-03-16Version 1

Recent observations of galactic cosmic rays (CR) in the 1-500 GeV energy range have revealed striking deviations from what deemed "standard." The anomalies cut across hadronic and leptonic CRs. I discuss findings that challenge physical mechanisms long held responsible for the CR production in galactic supernova remnants (SNR). I also consider some new physics of particle acceleration in SNR shocks that is not part of conventional models but may explain the anomalies. However, a possible 20-30\% excess remains unaccounted for in the $e^{+}/e^{+}$ ratio over the range of a few 100 GeV. If not explained by future models, it suggests an additional source of positrons such as a dark matter decay/annihilation or pulsar contribution. Earlier efforts to explain both the $e^{+}/e^{-}$ and $p$/He anomalies with the "standard" models by adjusting the SNR environmental parameters and multiple sources are critically assessed.

Comments: Cosmic Rays beyond the Standard Model, San Vito, 2016, http://www.crbtsm.eu/, conference paper
Categories: astro-ph.HE
Related articles: Most relevant | Search more
arXiv:1910.10168 [astro-ph.HE] (Published 2019-10-22)
Realistic modeling of wind and supernovae shocks in star clusters: addressing ${\rm ^{22}Ne/^{20}Ne}$ and other problems in Galactic cosmic rays
arXiv:1909.02908 [astro-ph.HE] (Published 2019-09-06)
Study on the 3D anisotropic propagation of Galactic cosmic rays
arXiv:1904.10220 [astro-ph.HE] (Published 2019-04-23)
Galactic Cosmic Rays after AMS-02