Speaker
Alberto Oliva
(CIEMAT)
Description
We compute the energy spectra of antideuterons and antihelium in cosmic rays in a scenario where hadronic interactions inside supernova remnants can produce a diffusively shock-accelerated “source component” of secondary antinuclei along with their standard secondary component expected from cosmic ray collisions in the interstellar gas.
Primary authors
Alberto Oliva
(CIEMAT)
Nicola Tomassetti
(INFN and University of Perugia)
