AMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark Matter

Apr 16, 2015
12 pages
Published in:
  • JCAP 09 (2015) 023
  • Published: Sep 8, 2015
e-Print:
Report number:
  • SACLAY-T13-137,
  • LAPTH-019-15,
  • LAPP-EXP-2015-01
Experiments:

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Abstract: (IOP)
Using the updated proton and helium fluxes just released by the AMS-02 experiment we reevaluate the secondary astrophysical antiproton to proton ratio and its uncertainties, and compare it with the ratio preliminarly reported by AMS-02. We find no unambiguous evidence for a significant excess with respect to expectations. Yet, some preference for a flatter energy dependence of the diffusion coefficient (with respect to the MED benchmark often used in the literature) starts to emerge. Also, we provide a first assessment of the room left for exotic components such as Galactic Dark Matter annihilation or decay, deriving new stringent constraints.
Note:
  • 12 pages, 5 figures; Comments and clarifications added (including an appendix), matches version published on JCAP
  • dark matter theory
  • cosmic ray theory
  • cosmic ray experiments
  • dark matter experiments
  • dark matter: annihilation
  • galaxy: dark matter
  • AMS
  • anti-p
  • energy dependence
  • diffusion