  Conformal gravity can elegantly solve the problem of spacetime singularities
present in Einstein's gravity. For every physical spacetime, there is an
infinite family of conformally-equivalent singularity-free metrics. In the
unbroken phase, every non-singular metric is equivalent and can be used to
infer the physical properties of the spacetime. In the broken phase, a
Higgs-like mechanism should select a certain vacuum, which thus becomes the
physical one. However, in the absence of the complete theoretical framework we
do not know how to select the right vacuum. In this paper, we study the energy
conditions of non-singular black hole spacetimes obtained in conformal gravity
assuming they are solutions of Einstein's gravity with an effective
energy-momentum tensor. We check whether such conditions can be helpful to
select the vacuum of the broken phase.
