  Two classes of metrics obtained from non-Riemannian gravitational collapse
are presented.The first is the Taub planar symmetric exact solutions of
Einstein-Cartan field equations of gravity describing torsion walls which are
obtained from gravitational collapse of time dependent perturbation of
Riemannian Taub symmetric solutions of General Relativity.The second is a
modification of the Vilenkin Riemannian planar wall which is obtained from a
non-Riemannian planar distribution of spinning matter.
