  From the Wheeler-Dewitt solutions, the scale factor of the initial universe
is discussed. In this study, scale factors from Wheeler-Dewitt solutions, loop
quantum gravity, and phantom energy dominated stages are compared. Certain
modifications have been attempted in scale factor and quantum potentials driven
by canonical quantum gravity approaches. Their results are discussed in this
work. Despite an increment of phantom energy density, avoidance of Big Rip is
reported. Scale factors predicted from various models are discussed in this
work. The relationship between scale factors and the smooth continuation of
Aeon is discussed by the application of conformal cyclic cosmology. Quantum
potentials for various models are correlated and a correction parameter is
included in the cosmological constant. Phantom energy dominated, final stage
non-singular evolution of the universe is found. Eternal increment of phantom
energy density without interacting with dark matter is reported for the
consequence of the evolution of the future universe. Also, the non-interacting
solutions of phantom energy and dark matter are explained. As the evolution
continues even after the final singularity is approached, the validity of
conformal cyclic cosmology is predicted. Non zero values for the scale factor
for the set of eigenvalues are presented. Results are compared with
supersymmetric classical cosmology. The non-interacting solutions are compared
with SiBI solutions
