15-19 September 2014
DESY Hamburg
Europe/Berlin timezone
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Contribution List

Displaying 19 contributions out of 19
Presented by Andi HEKTOR on 18 Sep 2014 at 9:30 AM
Presented by Daniel KÜMPEL on 16 Sep 2014 at 9:30 AM
Session: Student Talks
Light anti-nuclei, namely anti-deuteron and anti-helium, can be produced through the nuclear coalescence of the anti-protons and the anti-neutrons that are originated in a dark matter pair annihilation event. At low kinetic energies, the fluxes of these bound states are found to dominate over the astrophysical background and thus anti-nuclei may be considered as a very promising channel for a dark ... More
Presented by Mr. Andrea VITTINO on 19 Sep 2014 at 10:20 AM
on 19 Sep 2014 at 3:00 PM
on 15 Sep 2014 at 3:00 PM
on 16 Sep 2014 at 3:00 PM
on 17 Sep 2014 at 3:00 PM
on 18 Sep 2014 at 3:00 PM
Presented by Dario GRASSO on 15 Sep 2014 at 9:30 AM
Presented by Guenter SIGL on 15 Sep 2014 at 9:00 AM
Presented by Christoph WENIGER on 17 Sep 2014 at 9:30 AM
Presented by Carmelo EVOLI on 18 Sep 2014 at 11:30 AM
Session: Student Talks
An understanding of the origin of cosmic rays requires inferring source as well as propagation parameters from the analysis of the data. While it is well appreciated that propagation parameters depend on the propagation model adopted, it is also important to gauge to what extent they are affected by more or less implicit assumptions on the source properties. I present some results about such possi ... More
Presented by Mr. Yoann GÉNOLINI on 19 Sep 2014 at 10:40 AM
Session: Student Talks
Presented by Jie FENG on 19 Sep 2014 at 11:40 AM
Session: Student Talks
Presented by Mathieu BOUDAUD on 19 Sep 2014 at 11:20 AM
Presented by David WALZ on 16 Sep 2014 at 11:30 AM
Presented by Daniele GAGGERO on 15 Sep 2014 at 11:30 AM
Presented by Francesca CALORE on 17 Sep 2014 at 11:30 AM
Session: Student Talks
Dwarf spheroidal galaxies (dSph) are dominated dark matter (DM) astrophysical objects which allow us to put tight constraints on the velocity averaged annihilation cross-section of weakly interacting massive particles (WIMPs). Such bounds, coming from the observation of dSphs in the gamma-ray band, depend crucially on the mass modelling of this peculiar class of galaxies. We will review the momen ... More
Presented by Mr. Mauro VALLI on 19 Sep 2014 at 10:00 AM