We examine a real electroweak triplet scalar field as dark matter,
abandoning the requirement that its relic abundance is determined
through freeze out in a standard cosmological history (a situation which
we refer to as `miracle-less WIMP’). We extract the bounds on such a
particle from collider searches, searches for direct scattering with
terrestrial targets, and searches for the indirect products of
annihilation. Each type of search provides complementary information,
and each is most effective in a different region of parameter space. LHC
searches tend to be highly dependent on the mass of the SU(2) charged
partner state, and are effective for very large or very tiny mass
splitting between it and the neutral dark matter component. Direct
searches are very effective at bounding the Higgs portal coupling, but
ineffective once it falls below \lambda_{\text{eff}} \lesssim 10^{-3}λeff≲10−3.
Indirect searches suffer from large astrophysical uncertainties due to
the backgrounds and JJ-factors,
but do provide key information for \sim∼
100 GeV to TeV masses. Synthesizing the allowed parameter space, this
example of WIMP dark matter remains viable, but only in miracle-less
regimes.