  In this work, non perfect fluid, tilted source solutions in both
Einstein-Hilbert General Relativity (GR) and Quadratic Gravity (QG) for the
anisotropic Bianchi V model are addressed. Since the excellent CMBR match of
Starobinsky's inflation with Planck's team measurements data, QG has acquired a
prominent status in the effective sense, for sufficiently strong gravity
fields. The main interest is in the numeric time evolution to the past towards
the singularity and the behavior of the kinematic variables, vorticity,
acceleration, and the expansion of this source substance. In QG we found that
for universes with higher and smaller matter densities fall into the Kasner or
isotropic singularity attractors to the past, respectively. We also found that
the Kasner singularity attractor to the past has always zero vorticity, for
both GR and QG theories. While for QG the isotropic singularity attractor may
have divergent vorticity. For the set of assumptions and conditions supposed in
this work, the isotropic singularity attractor, favors QG as compared to GR.
Only in QG we were able to find a geometric singularity with divergences in all
of the kinematic variables of the substance, decreasing to finite values to the
future, upon time reversing. That is, we obtained an initial kinematic
singularity substance, that approaches a perfect fluid source.
