$\mathrm{\Psi }=\mathrm{W}{\mathrm{e}}^{\pm \mathrm{\Phi }}$ quantum cosmological solutions for Class A Bianchi Models

We find solutions for quantum Class A Bianchi models of the form $\rm \Psi=W e^{\pm \Phi}$ generalizing the results obtained by Moncrief and Ryan in standard quantum cosmology. For the II and IX Bianchi models there are other solutions ${\tilde{\mathrm{\Phi }}}_2$, ${\tilde{\mathrm{\Phi }}}_9$ to the Hamilton-Jacobi equation for which $\mathrm{\Psi }$ is necessarely zero, in contrast with solutions found in supersymmetric quantum cosmology.