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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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Multi-wavelength signals of dark matter annihilations at the Galactic center (15'+5')
 
I will present a study of the multi--wavelength signal induced by weakly
interacting massive particle (WIMP) annihilations at the Galactic Center.
Referring to a generic WIMP dark matter scenario and depending on
astrophysical inputs, I will discuss spectral and angular features and
sketch correlations among signals at different frequencies.
Data-sets at all energy bands, namely the radio, near infrared, X-ray and
gamma-ray bands, contribute to place significant constraints on the WIMP
parameter space.
The possibility of a dark matter discovery with the next generation of
gamma-ray telescopes, like GLAST and CTA, and with wide-field radio
observations, will be also briefly discussed.
 
Id: 379
Place: AlbaNova
Room: Oskar Klein auditorium
Starting date:
20-Aug-2008   16:55
Duration: 20'
Contribution type: Talk
Primary Authors: Mr. REGIS, Marco (S.I.S.S.A.)
Presenters: Mr. REGIS, Marco
Material: slide Slides
 
Included in session: Multi messenger searches and the galactic centre
Included in track: Multi messenger searches
 

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