The origin of high-energy cosmic rays, atomic nuclei that continuously impact Earth's
atmosphere, is unknown. Because of deflection by interstellar magnetic fields, cosmic rays …

We present version 2 of the DRAGON code designed for computing realistic predictions of
the CR densities in the Galaxy. The code numerically solves the interstellar CR transport …

We compute the γ-ray and neutrino diffuse emission of the Galaxy on the basis of a recently
proposed phenomenological model characterized by radially dependent cosmic-ray (CR) …

Astrophysical sources of neutrinos detected by large-scale neutrino telescopes remain
uncertain. While there exist statistically significant observational indications that a part of the …

We model the transport of cosmic ray nuclei in the galaxy by means of a new numerical
code. At variance with previous numerical models, ours accounts for a generic spatial …

The IceCube Collaboration has recently reported evidence for a high-energy extraterrestrial
neutrino flux. During two years of operation 28 events with energies between 30 TeV and …

High-energy neutrinos present the ultimate signature for a cosmic ray accelerator. Galactic
sources responsible for acceleration of cosmic ray up to the knee in cosmic ray spectrum will …

The origin of high-energy cosmic rays, and their behavior in astrophysical sources, remains
an open question. Recently, new ways to address this question have been made possible …

We use our numerical code, DRAGON, to study the implications of recent data on our
knowledge of the propagation properties of cosmic ray nuclei in the Galaxy. We show that …

We study the contribution of Galactic sources to the flux of astrophysical neutrinos recently
observed by the IceCube Collaboration. We show that in the simplest model of …