Is there an antiproton excess near 10 to 20 GeV?
In plain words
Some analyses of space-station data found slightly more antiprotons near 10 to 20 GeV than expected, which could come from dark matter particles annihilating. Others find the excess disappears when measurement errors and production rates are treated more carefully.
Precise statement
Decide whether the AMS-02 antiproton-to-proton ratio shows a statistically significant excess at rigidities of about 10 to 20 GV over secondary production, once correlated systematic errors, antiproton production cross-section uncertainties and solar modulation are included. A significant excess has been fit by dark matter of mass about 50 to 80 GeV annihilating to b-bbar.
What would settle it
Published AMS-02 correlation matrices plus new accelerator measurements of p-p and p-He antiproton production at the relevant energies.
Status in the literature
Unverified note: it names recent work and was partly written without a live literature search; it awaits a check by an editor.
Analyses including correlated errors reduced the significance below about $2\sigma$, and 2025 studies of solar modulation (Duan et al., JCAP, 2025) have not produced a consensus.
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