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Search for Dark Matter with IceCube (pptx)
If non-baryonic dark matter exists in the form of neutralinos, a neutrino flux is expected from the decay of neutralino pair annihilation products inside heavy celestial bodies, where these particles can be gravitationally trapped.

 

Handle: Document-57025
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Wednesday, February 16, 2011 09:02:24 AM CST
Wednesday, February 16, 2011 09:02:24 AM CST
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  • Search for Dark Matter with IceCube Catherine De Clercq for the IceCube Collaboration Vrije Universiteit Brussel w3.iihe.ac.be Outline Weakly Interacting Massive Particles as Cold Dark Matter The IceCube neutrino detector Search for neutrino signals of WIMP annihilations in the Sun and near the Galactic Centre IceCube + DeepCore : prospects for Dark Matter discovery in the coming years Catherine De Clercq DM in IceCube 2 Dark matter Evidence for Dark Matter from observations Indirect detection Catherine...
  • 0.21 WMAP Detection Catherine De Clercq DM in IceCube 6 Indirect detection Catherine De Clercq DM in IceCube 7 WIMP WIMP e+, ?, ?, p IceCube Mission Instrument Neutrino detection 8 ...
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Catherine De Clercq
Microsoft PowerPoint 2007 (.pptx) - application/vnd.openxmlformats-officedocument.presentationml.presentation
Presentation_DeClercq_forweb.pptx
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Appears In: Dark Matter in the LHC era
Preferred Version: Search for Dark Matter with IceCube (pptx)

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