We provide a statistical communication model for the phenomenon of quantum information evaporation from black holes (BHs). A BH behaves as a re°ecting quantum channel in a very special regime, which allows for a receiver to perfectly recover the absorbed quantum information. The quantum channel of a perfectly re°ecting (PR) BH is the probabilistically weighted sum of in¯nitely many qubit cloning channels. In this work, we reveal the statistical communication background of the information evaporation process of PR BHs. We show that the density of the cloned quantum particles in function of the PR BH's mass approximates a Chi-square distribution, while the stimulated emission process is characterized by zero-mean, circular symmetric complex Gaussian random variables. The results lead to the existence of Rayleigh random distributed coe±cients in the probability density evolution, which con¯rms the presence of Rayleigh fading (a special type of random°uctuation) in the statistical communication model of BH information evaporation.