  The vanishing of the Higgs quartic coupling at a high energy scale may be
explained by Intermediate Scale Supersymmetry, where supersymmetry breaks at
$(10^9$-$10^{12})$ GeV. The possible range of supersymmetry breaking scales can
be narrowed down by precise measurements of the top quark mass and the strong
coupling constant. On the other hand, nuclear recoil experiments can probe
Higgsino or sneutrino dark matter up to a mass of $10^{12}$ GeV. We derive the
correlation between the dark matter mass and precision measurements of standard
model parameters, including supersymmetric threshold corrections. The dark
matter mass is bounded from above as a function of the top quark mass and the
strong coupling constant. The top quark mass and the strong coupling constant
are bounded from above and below respectively for a given dark matter mass. We
also discuss how the observed dark matter abundance can be explained by
freeze-out or freeze-in during a matter-dominated era after inflation, with the
inflaton condensate being dissipated by thermal effects.
