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Galaxies clusters - PowerPoint PPT Presentation

Universal Matter : 20% Baryons (i.e. Protons, Neutrons and Electrons) 80% Dark Matter (???)

Girton College, Cambridge December 2008. The relative importance of the nature of DM is huge. Identify anomalous features in cosmic-ray spectra. Deduce constraints on Dark Matter properties by fitting to observations. Calculate local fluxes of DM annihilation/decay products.

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Galaxies clusters - PowerPoint PPT Presentation

Universal Matter : 20% Baryons (i.e. Protons, Neutrons and Electrons) 80% Dark Matter (???)