  We reconsider the study of the interior of the Schwarzschild black hole now
including inverse triad quantum corrections within loop quantization. We derive
these corrections and show that they are are related to two parameters
$\delta_b, \delta_c$ associated to the minimum length in the radial and angular
directions, that enter Thiemann's trick for quantum inverse triads.
Introduction of such corrections may lead to non-invariance of physical results
under rescaling of the fiducial volume needed to compute the dynamics, due to
noncompact topology of the model. So, we put forward two prescriptions to
resolve this issue. These prescriptions amount to interchange $\delta_b,
\delta_c$ in classical computations in Thiemann's trick. By implementing the
inverse triad corrections we found, previous results such as singularity
resolution and black-to-white hole bounce hold with different values for the
minimum radius-at-bounce, and the mass of the white hole.
