Name: CRATER 2018
Start: 2018-05-28T08:00:00+02:00
End: 2018-06-01T18:00:00+02:00
Location: Gran Sasso Science Institute

Alternative interpretations of secondary cosmic ray origin

Cosmic ray diffusion in Galactic magnetic field models

Cosmic ray diffusion in galactic turbulence

Cosmic ray propagation in molecular clouds

Cosmic ray transport in radiogalaxies and clusters

Cosmic Rays in the Galaxy: Closing remarks

Cosmic rays small-scale anisotropy

Cosmic-ray acceleration

Cosmic-ray induced galactic winds

Cosmic-ray large scale anisotropy

Cosmic-ray propagation at PeV energy and the interpretation of the cosmic-ray knee

Cosmic-ray transport from acceleration at SNRs to galactic scales

CR propagation near their sources

Difference between cosmic ray spectra in molecular clouds and in diffuse gas can explain the FERMI GeV excess

Discussion

Evidences of a hard cosmic ray population in the Galactic Center region and their possible interpretations

Experiments focusing on the cosmic-ray energy spectrum around the knee

Extended nearby VHE gamma-ray sources and the positron flux at the Earth

Imprints of cosmic rays in multifrequency observations of the interstellar emission

Magnetohydrodynamic turbulence and the role of intermittent structures

Measurements of nuclear cross-sections at CERN SPS.

Non-linear cosmic ray transport

Observations of the interstellar magnetic turbulence

Opening talk: Theory and Interpretation of Galactic Cosmic Rays

Possible explanations of the recent galactic cosmic-ray anomalies

Production of secondaries in Galactic cosmic rays

Recent developments and results obtained with the USINE code

Recent developments of the PICARD code

Recent results of the AMS-02 experiments

CRATER 2018

Material Package