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:
- 1504.04276 [astro-ph.HE]
Report number:
- SACLAY-T13-137,
- LAPTH-019-15,
- LAPP-EXP-2015-01
Experiments:
View in:
Citations per year
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
References(58)
Figures(12)
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