  We study the formation and the evaporation of a spherically symmetric black
hole in conformal gravity. From the collapse of a spherically symmetric thin
shell of radiation, we find a singularity-free non-rotating black hole. This
black hole has the same Hawking temperature as a Schwarzschild black hole with
the same mass, and it completely evaporates either in a finite or in an
infinite time, depending on the ensemble. We consider the analysis both in the
canonical and in the micro-canonical statistical ensembles. Last, we discuss
the corresponding Penrose diagram of this physical process.
