  The dynamics of the vacuum Kantowski-Sachs space-time are studied in the
so-called limiting curvature mimetic gravity theory. It is shown that in this
theory the vacuum Kantowski-Sachs space-time is always singular. While the
departures from general relativity due to the limiting curvature mimetic theory
do provide an upper bound on the magnitude of the expansion scalar, both its
rate of oscillations and the magnitude of the directional Hubble rates increase
without bound and cause curvature invariants to diverge. Also, since the radial
scale factor does not vanish in finite (past) time, in this particular theory
the Kantowski-Sachs space-time cannot be matched to a null black hole event
horizon and, therefore, does not correspond to the interior of a static and
spherically symmetric black hole.
