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Dark Matter signal from $\mathrm{e^{+}/e^{-}/\bar{p}}$ with the AMS-02 Detector on the International Space Station
The excess of the antiproton flux and the antiproton-to-proton flux ratio beyond the prediction of the collision of ordinary cosmic rays is a unique signal from dark matter models of neutralino annihilation. This excess cannot come from pulsars. We present precision measurements by AMS-02 of the ant...
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| Lenguaje: | eng |
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SISSA
2017
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| Acceso en línea: | https://dx.doi.org/10.22323/1.314.0090 http://cds.cern.ch/record/2838145 |