  A recently proposed dark matter WIMP has only second-order couplings to gauge
bosons and itself. As a result, it has small annihilation, scattering, and
creation cross-sections, and is consequently consistent with all current
experiments and the observed abundance of dark matter. These cross-sections
are, however, still sufficiently large to enable detection in experiments that
are planned for the near future, and definitive identification in experiments
proposed on a longer time scale. The (multi-channel) cross-section for
annihilation is consistent with thermal production and freeze-out in the early
universe, and with current evidence for dark matter annihilation in analyses of
the observations of gamma rays by Fermi-LAT and antiprotons by AMS-02, as well
as the constraints from Planck and Fermi-LAT. The cross-section for direct
detection via collision with xenon nuclei is estimated to be slightly below
$10^{-47}$ cm$^2$, which should be attainable by LZ and Xenon nT and well
within the reach of Darwin. The cross-section for collider detection via vector
boson fusion is estimated to be $\sim 1$ fb, and may be ultimately attainable
by the high-luminosity LHC; definitive collider identification will probably
require the more powerful facilities now being proposed.
