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We derive limits on the dark matter annihilation cross section and lifetimeusing measurements of the AMS-02 antiproton ratio and positron fraction data.In deriving the limits, we consider the scenario of secondary particlesaccelerated in supernova remnants (SNRs) which has been argued to be able toreasonably account for the AMS-02 high energy positron/antiproton fractiondata. We parameterize the contribution of secondary particles accelerated inSNRs and then fit the observational data within the conventional cosmic raypropagation model by adopting the GALPROP code. We use the likelihood ratiotest to determine the 95$\%$ confidence level upper limits of the possible darkmatter (DM) contribution to the antiproton/positron fractions measured byAMS-02. Our limits are stronger than that set by the Fermi-LAT gamma-ray Pass 8data of the dwarf spheroidal satellite galaxies. We also show that the solarmodulation (cosmic ray propagation) parameters can play a non-negligible rolein modifying the constraints on the dark matter annihilation cross section andlifetime for $m_\chi<100$ GeV ($m_\chi>100$ GeV), where $m_\chi$ is the restmass of the dark matter particles. Using this results, we also put limits onthe effective field theory of dark matter.

Limits on the Dark Matter from AMS-02 antiproton and positron fraction data