Handling the Uncertainties in the Galactic Dark Matter Distribution for Particle Dark Matter Searches

11 Jun 2019 Benito Maria Cuoco Alessandro Iocco Fabio

In this work we characterize the distribution of Dark Matter (DM) in the Milky Way (MW), and its uncertainties, adopting the well known "Rotation Curve" method. We perform a full marginalization over the uncertainties of the Galactic Parameters and over the lack of knowledge on the morphology of the baryonic components of the Galaxy... (read more)

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Categories


  • ASTROPHYSICS OF GALAXIES
  • HIGH ENERGY PHYSICS - PHENOMENOLOGY