Le 8 décembre 2017
De 10h30 à 12h00
Martin Stref
Montpellier
The particle dark matter scenario is currently being probed by direct and indirect searches experiments. Making prediction for these experiments requires a knowledge of the Galactic dark matter phase space (mass density and velocity distribution of the dark matter particles). Modeling the small-scale structuring of the dark halo is especially important in this context. I will present methods to model this structuring, as well as the full Galactic phase space, while remaining consistent with known dynamical constraints.