$\rm Ψ= W e^{\pm Φ}$ quantum cosmological solutions for Class A Bianchi Models
We find solutions for quantum Class A Bianchi models of the form $\rm Ψ=W e^{\pm Φ}$ generalizing the results obtained by Moncrief and Ryan in standard quantum cosmology. For the II and IX Bianchi models there are other solutions $\rm \tildeΦ_2$, $\rm \tildeΦ_9$ to the Hamilton-Jacobi equation for which $\rm Ψ$ is necessarely zero, in contrast with solutions found in supersymmetric quantum cosmology.
gr-qc↗