Speakers
Nicola Tomassetti
(Perugia University & INFN- Perugia)
Alberto Oliva
(Centro de Investigaciones Energéti cas Medioambientales y Tecno)
Description
Antimatter nuclei in cosmic rays (CRs) represent a promising tool for the indirect search of dark-matter particles in the Galaxy.
At this conference, we report updated calculations for the astrophysical production of CR antiproton, antideuteron, and antihelium nuclei using updated cross-section formulae and new astrophysical constraints inferred from the recent AMS-02 data on CR protons and nuclei. Using these constraints, we also compute upper limits for the flux of CR antinuclei produced and diffusively-shock-accelerate inside Galactic sources.
Author
Nicola Tomassetti
(Perugia University & INFN- Perugia)