2009/04/07 by Carolin B. Braeuninger, Carolin Barbara Bräuninger, Marco Cirelli · 1 citation
Physics and Astronomy · #Annihilation #Astrophysics #Boson #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Dark matter halo #Deuterium #Galactic halo #Galaxy #Gauge boson #Gauge theory #Halo #Light dark matter #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Range (aeronautics) #Scalar field dark matter #Weakly interacting massive particles #hep-ph
paper · pdf · doi:10.1016/j.physletb.2009.05.059
published as Phys.Lett.B678:20-31,2009 · 17 pages, 6 figures
arxiv created 2009/04/07 · openalex publication_date 2009/05/30 · arxiv updated 2010/12/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We study the fluxes of anti-deuterons that could be produced by annihilations in the galactic halo of Dark Matter particles with multi-TeV mass and a large annihilation cross section, as indicated by the recent PAMELA results. The model of Minimal Dark Matter (MDM) is an example in this category. We find that the fluxes are well within the reach of planned experiments for DM candidates that annihilate mainly into quark pairs, and also extend into the multi-GeV range above the background. They are instead suppressed and concentrated at too large energies to emerge above the background if the main annihilation channel is into gauge bosons (such as in particular W+W- in the MDM case).