The properties of canonical and microcanonical ensembles of a black hole with thermal radiation and the problem of black hole evaporation in 3-D are studied. In 3-D Einstein-anti-de Sitter gravity we have two relevant mass scales, mc = 1/G, and mp = (h̄ Λ/G)1/3, which are particularly relevant for the evaporation problem. It is argued that in the ‘weak coupling’ regime Λ < (h̄G)−2, the end point ...