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We present novel constraints on cosmic-ray propagation in the Galaxy using the recent precise measurements of proton and helium spectra from AMS-02, together with preliminary AMS-02 data on the antiproton over proton ratio.
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Andrew W. Strong, Igor V. Moskalenko, and Vladimir S. Ptuskin · 2007
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Possible physics scenarios behind cosmic-ray "anomalies"
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O. Adriani et al · 2011
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R. Trotta, G. Johannesson, I. V. Moskalenko, T. A. Porter, R. Ruiz de Austri, and A. W. Strong · 2011
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Cosmic-Ray Proton and Helium Spectra from the First CREAM Flight
Y. S. Yoon et al · 2011
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Solar modulation parameter for cosmic rays since 1936 reconstructed from ground-based neutron monitors and ionization chambers
Ilya G. Usoskin, Galina A. Bazilevskaya, and Gennady A. Kovaltsov · 2011
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Testing the Origin of High-Energy Cosmic Rays
Andrey E. Vladimirov, Gudlaugur Johannesson, Igor V. Moskalenko, and Troy A. Porter · 2012
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Spectral breaks as a signature of cosmic ray induced turbulence in the Galaxy
Pasquale Blasi, Elena Amato, and Pasquale D. Serpico · 2012
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Nonlinear cosmic ray Galactic transport in the light of AMS-02 and Voyager data
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Carmelo Evoli, Daniele Gaggero, and Dario Grasso · 2015
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A. W. Strong · 2015
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Solar Modulation of the Proton Local Interstellar Spectrum with AMS-02, Voyager 1 and PAMELA
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Cosmic-ray diffusive reacceleration: a critical look
Luke O’C. Drury and Andrew W. Strong · 2015
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Bayesian analysis of cosmic-ray propagation: evidence against homogeneous diffusion
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