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Integrability of classical strings in the BTZ black hole enables theconstruction and study of classical string propagation in this background. Wefirst apply the dressing method to obtain classical string solutions in the BTZblack hole. We dress time like geodesics in the BTZ black hole and obtain openstring solutions which are pinned on the boundary at a single point and whoseend points move on time like geodesics. These strings upon regularising theircharge and spins have a dispersion relation similar to that of giant magnons.We then dress space like geodesics which start and end on the boundary of theBTZ black hole and obtain minimal surfaces which can penetrate the horizon ofthe black hole while being pinned at the boundary. Finally we embed the giantgluon solutions in the BTZ background in two different ways. They can beembedded as a spiral which contracts and expands touching the horizon or aspike which originates from the boundary and touches the horizon.

Generating string solutions in BTZ