9:00 AM
|
Galactic Cosmic Ray data
-Prof.
Fiorenza Donato
(Torino University)
(until 9:50 AM)
|
9:00 AM
|
Selected DAMPE results [15'+10']
-
Andrii Tykhonov
(Universite de Geneve (CH))
|
9:25 AM
|
Future precision experiments in CRs [15'+10']
-
Alberto Oliva
(Universita e INFN, Bologna (IT))
|
9:50 AM
|
Relevant XS reactions and precision for GCRs
-Prof.
Fiorenza Donato
(Torino University)
(until 11:05 AM)
|
9:50 AM
|
Deuteron and Helium-3 production cross sections and propagation in the Galaxy [10'+5']
-
Diego Mauricio Gomez Coral
(Universidad Nacional Autonoma (MX))
|
10:05 AM
|
Measurement of proton spallation cross-sections of natCr and 55Mn between 0.2-2.5 GeV relevant to galactic cosmic ray propagation [10'+5']
-
Priyarshini Ghosh
(NASA Goddard Space Flight Center)
|
10:20 AM
|
The Fluka cross sections for secondary cosmic rays: Latest results [10'+5']
-
Pedro De la Torre Luque
(Institute of theoretical physics (IFT-UAM))
|
10:35 AM
|
Data-driven constraints on cosmic-ray diffusion: Probing self-generated turbulence in the Milky Way [10'+5']
-
Alessandro Cuoco
|
10:50 AM
|
From the AMS-02 isotope fluxes to their production cross sections [10'+5']
-
Meng-Jie Zhao
(Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences)
|
11:05 AM
|
--- Coffee break - TH common room ---
|
11:30 AM
|
Brainstorming on a roadmap: preparing a white paper
(until 12:05 PM)
|
11:30 AM
|
Organisation to write white paper [30']
- Prof.
Fiorenza Donato
(Torino University)
Saverio Mariani
(CERN)
David Alain Maurin
(Centre National de la Recherche Scientifique (FR))
|
12:00 PM
|
Concluding remarks [5']
- Prof.
Fiorenza Donato
(Torino University)
|