Name: Cosmic ray backgrounds in dark matter searches
Start: 2010-01-25T09:00:00+01:00
End: 2010-01-27T22:20:00+01:00
Location: AlbaNova

Cosmic ray backgrounds in dark matter searches

from Monday, 25 January 2010 (09:00) to Wednesday, 27 January 2010 (22:20)

Monday, 25 January 2010
09:00
09:00 - 09:45
Room: Rotunda
Contributions

09:00 Registration
09:45
09:45 - 09:50
Room: FB54
Contributions

09:45 Edsjö - Welcome
09:50
09:50 - 10:00
Room: FB54
Contributions

09:50 Bergström - Introduction
10:00
10:00 - 13:00
Room: FB54
Contributions

10:00 Egberts - HESS electrons measurement(40' + 10')

10:50 Latronico - Cosmic-ray electrons with Fermi-LAT (40' + 10')

12:10 Boezio - PAMELA, an overview (40' + 10')
13:00 Lunch break
Lunch break
13:00 - 14:30
Room: Entré Restaurant
14:30
14:30 - 19:00
Room: FB54
Contributions

14:30 Wu - The cosmic-ray antiproton flux measured by PAMELA (20' + 10')

15:00 Mocchiutti - PAMELA electrons and positrons mesurement(20' + 10')

15:30 Gillard - PAMELA capability for Cosmic-Ray Mapping (20' + 10')

16:30 Mazziotta - Study of Cosmic Ray Electron Anisotropies with the Fermi-LAT data (20' + 10')

17:00 Zehr - PEBS measurement (20' + 10')

17:30 Putze - Energy spectra of cosmic-ray nuclei at high energies measured by CREAM (20' + 10')

18:00 Discussion (Boezio, Egberts, Latronico, de Angelis)
Tuesday, 26 January 2010
09:00
09:00 - 12:50
Room: FB54
Contributions

09:00 Maurin - Cosmic ray propagation (40' + 10')

09:50 Strong - Galprop and Diffuse gamma-ray emission / Fermi (40' + 10')

11:10 Maccione - Recent results on the propagation of high energy cosmic ray nuclei and antiprotons (30' + 10')

11:50 Delahaye - Theoretical uncertainties of the astrophysical electron flux at the Earth (20' + 10')

12:20 Putze - A MCMC technique to sample transport and source parameters of Galactic cosmic rays (20' + 10')
12:50 Lunch break
Lunch break
12:50 - 14:20
Room: Entré Restaurant
14:20
14:20 - 18:50
Room: FA32
Contributions

14:20 Bregeon - Fermi pulsar results and their implications (30' + 10')

15:00 Serpico - Pulsar models and electron/positron primary production (40' + 10')

15:50 Bucciantini - pulsars/magnetars (20' + 10')

16:50 Piran - Inhomogeneities in the SNR distribution as the origin of the PAMELA anomaly (20' + 10')

17:20 Mertsch - Cosmic ray acceleration in supernova remnants and the FERMI/PAMELA data (20' + 10')

17:50 Discussion (Maurin, Strong, Maccione)
19:00

19:00 - 21:30
Room: Entré Restaurant
Wednesday, 27 January 2010
10:00
10:00 - 12:40
Room: FP41
Contributions

10:00 Donato - e+/e- and pbar dark matter interpretation (40' + 10')

10:50 Ullio - Multimessengers and DM interpretation (40' + 10')

12:10 Gaggero - Possible Interpretations of the electron+positron spectrum measured by Fermi-LAT (20' + 10')
12:40 Lunch break
Lunch break
12:40 - 14:10
Room: Entré Restaurant
14:10
14:10 - 17:20
Room: FP41
Contributions

14:10 Gondolo - Axions (30' + 10')

14:50 de Angelis - MAGIC constraints on axions (20' + 10')

15:20 Cuoco - Multiwavelength Dark Matter constraints (20' + 10')

16:20 Discussion (Donato, Ullio, Gondolo)
17:20 Summary Talk - Edsjö
Summary Talk - Edsjö
17:20 - 17:50
Room: FP41