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We propose a description of how a large, cold black hole (black zero-brane)in type IIA superstring theory evaporates into freely propagating D0-branes, bysolving the dual gauge theory quantitatively. The energy spectrum of emittedD0-branes is parametrically close to thermal when the black hole is large. Theblack hole, while initially cold, gradually becomes an extremely hot andstringy object as it evaporates. As it emits D0-branes, its emission ratespeeds up and it evaporates completely without leaving any remnant. Hence thissystem provides us with a concrete holographic description of black holeevaporation without information loss.

A microscopic description of black hole evaporation via holography