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The Indirect Detection of Non-Baryonic Dark Matter

The Indirect Detection of Non-Baryonic Dark Matter. Application for a Postdoctoral Research Fellowship with the Science And Technology Research Council. Dr. Daniel T. Cumberbatch Case Western Reserve University. Universal Matter Constituents. 80 % DARK MATTER. 20% Baryons.

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278 views • 14 slides

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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148 views • 2 slides

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Constrain dm - PowerPoint PPT Presentation

The Indirect Detection of Non-Baryonic Dark Matter

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