Constraining Dark Matter models with antiprotons
Since the discovery of the first ‘negative proton’ in 1955, antiprotons have become a fundamental pillar in experimental high-energy physics, both in collider physics and astrophysics. par In this seminar I will show how to extract bounds on Dark Matter models using our current understanding of the cosmic-ray antiproton flux measured by the PAMELA experiment.
SISSA
Speaker
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Alfredo Urbano
