AMS-02 beryllium data and its implication for cosmic ray transport

10 Jan 2020 Evoli Carmelo Morlino Giovanni Blasi Pasquale Aloisio Roberto

The flux of unstable secondary cosmic ray nuclei, produced by spallation processes in the interstellar medium, can be used to constrain the residence time of cosmic rays inside the Galaxy. Among them, $^{10}$Be is especially useful because of its relatively long half-life of 1.39 Myr... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA