  Dark sectors with strong interactions have received considerable interest.
Assuming the existence of a minimally coupled dark sector which runs to strong
interactions in the infrared, we address the question whether the scaling
behavior of this dark sector can be observed in missing energy signatures at
present and future hadron colliders. We compare these findings to the concrete
case of self-interacting dark matter and demonstrate that the energy dependence
of high-momentum transfer final states can in principle be used to gain
information about the UV structure of hidden sectors at future hadron
colliders, subject to large improvements in systematic uncertainties, which
could complement proof-of-principle lattice investigations. We also comment on
the case of dark Abelian $U(1)$ theories.
