  We propose a new selection criteria for predicting the most probable
wavefunction of the universe that propagates on the string landscape
background, by studying its dynamics from a quantum cosmology view. Previously
we applied this proposal to the $SUSY$ sector of the landscape. In this work
the dynamic selection criterion is applied to the investigation of the
non-$SUSY$ sector.In the absence of detailed information about its structure,
it is assumed that this sector has a stochastic distribution of vacua
energies.The calculation of a distribution probability for the cosmological
constants $\Lambda_{eff}$, obtained from the density of states $\rho$,
indicates that the most probable wavefunction is peaked around universes with
zero $\Lambda_{eff}$. In contrast to the {\it extended wavefunction} solutions
found for the $SUSY$ sector with $N$-vacua and peaked around
$\Lambda_{eff}\simeq \frac{1}{N^2}$, wavefunctions residing on the non-$SUSY$
sector exhibit {\it Anderson localization}.Although minisuperspace is a limited
approach it presently provides a dynamical quantum selection rule for the most
probable vacua solution from the landscape.
