  Models with a tiny coupling $\lambda$ between the dark matter and the
Standard Model, $\lambda \sim v/M_\text{Pl}\sim 10^{-16}$, can yield the
measured relic abundance through the thermal process known as freeze-in. We
propose to interpret this small number in the context of perturbative large $N$
theories, where couplings are suppressed by inverse powers of $N$. Then $N \sim
M_{\rm Pl}^2/v^2$ gives the observed relic density. Additionally, the ultimate
cutoff of the Standard Model is reduced to $\sim 4\,\pi\, M_\text{Pl}/\sqrt{N}
\sim 4\, \pi\, v$, thereby solving the electroweak hierarchy problem. These
theories predict a direct relation between the Standard Model cutoff and the
dark matter mass, linking the spectacular collider phenomenology associated
with the low gravitational scale to the cosmological signatures of the dark
sector. The dark matter mass can lie in the range from hundreds of keV to
hundreds of GeV. Possible cosmological signals include washing out power for
small scale structure, indirect detection signals from dark matter decays, and
a continuous injection of electromagnetic and hadronic energy throughout the
history of the Universe.
