Abstract
Several studies have pointed out an excess in the AMS-02 antiproton spectrum
at rigidities of 10-20 GV. Its spectral properties were found to be consistent
with a dark-matter particle of mass 50-100 GeV which annihilates hadronically
at roughly the thermal rate. In this work, we reinvestigate the antiproton
excess including all relevant sources of systematic errors. Most importantly,
we perform a fully realistic derivation of the correlations in the AMS-02
systematic error which could potentially "fake" a dark-matter signal. The
dominant systematics in the relevant rigidity range originate from
uncertainties in the cross sections for absorption of cosmic rays within the
detector material. For the first time ever, we calculate their correlations
within the full Glauber-Gribov theory of inelastic scattering. The AMS-02
correlations enter our spectral search for dark matter in the form of
covariance matrices which we make publicly available for the cosmic-ray
community. We find that the global significance of the antiproton excess is
reduced to below 1 $\sigma$ once all systematics, including the derived AMS-02
error correlations, are taken into account. No significant preference for a
dark-matter signal in the AMS-02 antiproton data is found in the mass range
10-10000 GeV.
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