Prsentation PowerPoint

1
(No Transcript)
2
Outlook of the lectures
3
(No Transcript)
4
Françoise Combes
5
(No Transcript)
6
(No Transcript)
7
James Bartlett
8
(No Transcript)
9
(No Transcript)
10
Richard Taillet
11
(No Transcript)
12
(No Transcript)
13
(No Transcript)
14
Julien Lesgourgues
15
Gilbert Moultaka
16
(No Transcript)
17
(No Transcript)
18
(No Transcript)
19
(No Transcript)
20
A comparison between the same dark matter halo
simulated with 1 million particles (left panel)
and 8 million particles (right panel)
21
Ben Moore
22
Stefano Scopel
Q
23
(No Transcript)
24
Maryvonne De Jesus
25
(No Transcript)
26
(No Transcript)
27
(No Transcript)
28
(No Transcript)
29
F. Donato et al.
Uncertainties resulting from the CR propagation
model
30
(No Transcript)
31
David Maurin
32
Aurélien Barrau
33
(No Transcript)
34
(No Transcript)
35
HESS and Sagittarius A
Gianfranco Bertone
36
Up-going muons lose 1 GeV as they cross 4 meters
of ice or water The fiducial volume for the
neutrino-muon conversion increases with the
neutrino energy
37
Fabrice Feinstein
38
Satellite experiments
Sylvie Rosier
39
Corinne Goy
40
Comparison among the various signals
Jean Orloff
41
Spectre SPI des régions centrales de la Galaxie
Daprès Jean et al., AA 407, L55, 2003
42
Carte 511 keV des régions centrales de la Galaxie
FWHM 9 (-3 / 7)
Daprès Weidenspointner et al., Astro-ph / 0406178
43
Identification avec le bulbe galactique
Céline Boehm