Current status and future perspective in Cosmic-ray physics
by
Daniele Gaggero(SISSA, Trieste)
→
Europe/Berlin
Building 67, SemRm 10 (DESY Hamburg)
Building 67, SemRm 10
DESY Hamburg
Description
I will present a detailed introduction about the physics of CR propagation in the Galaxy and the open problems in this research field, with particular emphasis on the very accurate measurements published in the latest years and their implications. I will then describe in detail several results obtained with the DRAGON numerical package; in particular I will focus on the the importance of a realistic three-dimensional modeling of the Galaxy, and on the impact of the large and small scale Galactic strucutres on most CR observables. At the end I will stress the importance of a multi-messenger approach to CR physics, describing the role of gamma and radio observations, and I'll briefly point out future projects involving a deep interplay with other related research fields (turbulence, plasma physics).