On the origin of the GCR composition, in the light of the Ne22 excess

2 mars 2022, 14:15
45m
454A (salle Luc Valentin) (APC)

454A (salle Luc Valentin)

APC

Bâtiment Condorcet 10 rue Alice Domon et Léonie Duquet 75013 Paris

Orateur

Nikos Prantzos (IAP Paris)

Description

I will discuss the source composition of GCR and the implications for their acceleration site, emphasizing the role of the observed Ne22/Ne20 excess and the observed evolution of the light elements Li, Be and B , produced by GCR spallation reactions.

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