Starting with an asymptotically free gauge theory with dynamical symmetry breaking and a mass hierarchy, we investigate the Adler-Zee formula for the induced gravitational constant. We study the two-point function $\ensuremath{\psi}({q}^{2})$, constructed with the trace of the energy-momentum tensor. First, we show that if the zeros of $\ensuremath{\psi}$ are at a mass scale significantly below the leading scale, then ${{G}_{\mathrm{ind}}}^{\ensuremath{-}1}=O({{m}_{\mathrm{zero}}}^{2})$ making it impossible to get a realistic ${G}_{\mathrm{ind}}$ from the Adler-Zee formula with low-mass zeros. Next we use the Jensen formula to derive a sum rule for $|{m}_{\mathrm{zero}}|$. The analysis of this sum rule coupled with the result above leads to a dilemma with only one reasonable resolution. To get a realistic ${G}_{\mathrm{ind}}$ from the Adler-Zee formula, $\ensuremath{\psi}({q}^{2})$ must have a pair of complex-conjugate zeros at ${q}^{2}={{M}_{0}}^{2}\ifmmode\pm\else\textpm\fi{}2i\ensuremath{\gamma}{M}_{0}$, where ${M}_{0}$ is large and of the maximal scale and $\frac{\ensuremath{\gamma}}{{M}_{0}}\ensuremath{\ll}1$. The presence of this zero essentially determines ${{G}_{\mathrm{ind}}}^{\ensuremath{-}1}$. It gives a lower bound, which with our previously derived general upper bound gives $[\frac{{\ensuremath{\pi}}^{2}}{4(\mathrm{ln}10)288}]{C}_{\ensuremath{\psi}}{{M}_{0}}^{2}\ensuremath{\le}{(16\ensuremath{\pi}G)}^{\ensuremath{-}1}\ensuremath{\le}[\frac{5{\ensuremath{\pi}}^{2}}{288}]{C}_{\ensuremath{\psi}}{{M}_{0}}^{2}$, where ${C}_{\ensuremath{\psi}}$ is the anomaly coefficient, a number easily determined by low-order perturbation theory for any group.