activity
20072026
most citedStrong evidences of hadron acceleration in Tycho's Supernova Remnant

277 citations · 3.5k across the 94 of their papers we have counts for

collaborators
Showing 2019Show all

6 papers · 1 filter

astro-ph.HE2019★ 61 cited

Contribution of starburst nuclei to the diffuse gamma-ray and neutrino flux

Enrico Peretti, Pasquale Blasi, Felix Aharonian +2

In nuclei of starburst galaxies, the combination of an enhanced rate of supernova explosions and a high gas density suggests that cosmic rays can be efficiently produced, and that…

astro-ph.HE2019★ 119 cited

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

Carmelo Evoli, Giovanni Morlino, Pasquale Blasi +1

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…

astro-ph.HE2019★ 65 cited

Exploring particle escape in supernova remnants through gamma rays

Silvia Celli, Giovanni Morlino, Stefano Gabici +1

The escape process of particles accelerated at supernova remnant (SNR) shocks is one of the poorly understood aspects of the shock acceleration theory. Here we adopt a phenomenolog…

astro-ph.HE2019★ 108 cited

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +389

Neutrinos with energies above eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos…

astro-ph.HE2019★ 54 cited

Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +389

With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between eV and eV from point-like sources across the…

astro-ph.HE2019★ 24 cited

Effects of reacceleration and source grammage on secondary cosmic rays spectra

Virginia Bresci, Elena Amato, Pasquale Blasi +1

The ratio between secondary and primary cosmic ray particles is the main source of information about cosmic ray propagation in the Galaxy. Primary cosmic rays are thought to be acc…