$\rm Ψ= W e^{\pm Φ}$ quantum cosmological solutions for Class A Bianchi Models

Details $\rm Ψ= W e^{\pm Φ}$ quantum cosmological solutions for Class A Bianchi Models $\rm Ψ= W e^{\pm Φ}$ quantum cosmological solutions for Class A Bianchi Models

1995-06-08

arxiv.org/abs/gr-qc/9506021v1

Int.J.Theor.Phys. 35 (1996) 1381-1388

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

15 pages, Latex

Scientific paper

10.1007/BF02084947

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 $\rm \tilde\Phi_2$, $\rm \tilde\Phi_9$ to the Hamilton-Jacobi equation for which $\rm \Psi$ is necessarely zero, in contrast with solutions found in supersymmetric quantum cosmology.

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