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