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Hunt for dark matter using cosmic-ray antideuterons PvD€¦ · Diff. Halo Galactic Diffusion Coefficient Reference Model 0.01 Thickness 1 < L/kpc < Wind v —O km/s 0.3 cm /s Solar

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Page 1: Hunt for dark matter using cosmic-ray antideuterons PvD€¦ · Diff. Halo Galactic Diffusion Coefficient Reference Model 0.01 Thickness 1 < L/kpc < Wind v —O km/s 0.3 cm /s Solar

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Page 2: Hunt for dark matter using cosmic-ray antideuterons PvD€¦ · Diff. Halo Galactic Diffusion Coefficient Reference Model 0.01 Thickness 1 < L/kpc < Wind v —O km/s 0.3 cm /s Solar

P. von Doetinchem Antideuteron 2014 June 14 - p2p.

Discussion● More exchange between theory and experiments:

Start a community effort to use the best available models and sensitivities

● What experimental data are needed? What would we need from the collider community?

● framework for numerical propagation following AMS data relaease for heavynuclei

● constrain uncertainties: