  New non trivial solutions to the Lorentzian-signature symmetry reduced
Bianchi VIII Wheeler DeWitt equation for Hartle Hawking ordering parameters $
\pm 2\sqrt{33} $ are obtained using an Euclidean-signature semi classical
method. Using the aforementioned method we define 'excited' states for the
Bianchi VIII wave function and construct leading order 'excited' states which
appear to be a hybrid of scattering and bound states. Also six new solutions
for the $\Lambda \ne 0$ Bianchi VIII Euclidean-signature Hamilton Jacobi
equation are presented which can be used to construct semi-classical states
corresponding to the Lorentzian signature symmetry reduced Wheeler DeWitt
equation. In addition, new solutions to the Euclidean-signature Hamilton Jacobi
equation for the Bianchi VIII models are found when $\Lambda \ne 0$ and an
aligned primordial magnetic field is present. Furthermore, we find eight new
complex solutions to the Euclidean-signature Hamilton Jacobi equation for the
case when matter is not present, which can be used to construct additional
semi-classical states. We also study the leading order wave functions which
result from our aforementioned solutions when they are restricted to the
$\beta+$ axis. Prior to presenting these results we explain the
Euclidean-signature semi classical method and discuss how to solve the
resultant equations this method generates when it is applied to the
Lorentzian-signature symmetry reduced Bianchi VIII Wheeler DeWitt equation. The
Euclidean-signature semi-classical method used here is applicable to other
field theories as well. The work presented throughout this paper further shows
the power Eulclidean-signature semi classical methods possess for solving
problems in quantum cosmology and solving Lorentzian signature problems in
general.
