Back to Basics?... or How can supersymmetry be used in simple quantum cosmological model

The general theory of N=1 supergravity with supermatter is applied to a Bianchi type IX diagonal model. The supermatter is constituted by a complex scalar field and its spin-$\frac{1}{2}$ fermionic partners. The Lorentz invariant Ansatz for the wave function of the universe, $\mathrm{\Psi }$, is taken to be as simple as possible in order to obtain {\it new} solutions. The wave function has a simple form when the potential energy term is set to zero. However, neither the wormhole or the Hartle-Hawking state could be found. The Ansatz for $\mathrm{\Psi }$ used in this paper is constrasted with the more general framework of R. Graham and A. Csord'as.