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IDM2008 - Identification of Dark Matter 2008
IDM2008 - Identification of Dark Matter 2008
18-22 August 2008 AlbaNova
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Annihilation radiation predictions from N-body simulations (20'+5')
 
In the beginning of my talk I will present very recent results for the biggest
Milky-way sized halo simulation done so far. I will report on dark matter
annihilation predictions based on this simulation. The second part of the talk will
cover the influence of fine-grained phase-space caustics on the diffuse gamma 
ray
emission. The relevant scales cannot be covered by any state-of-the-art 
simulation.
Therefore I will introduce a new technique resolving the relevant scales and 
report
on the boost of diffuse emission due to these fine-grained caustics for simplified
halo models.
 
Id: 423
Place: AlbaNova
Room: Oskar Klein auditorium
Starting date:
18-Aug-2008   14:00
Duration: 25'
Contribution type: Talk
Primary Authors: Mr. VOGELSBERGER, Mark (MPA Garching, Germany)
Presenters: Mr. VOGELSBERGER, Mark
Material: slide Slides
 
Included in session: Indirect searches - gammas
Included in track: Indirect searches - gammas
 

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