A black hole in two-dimensional space-time

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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12 pages, Revtex, 2 figures

Scientific paper

An imploding shell of radiation is shown to create a 2-D black hole within the framework of the ``R=T'' theory. The radius of the horizon is given by 1/(2M), where M is the mass of the black hole. The topology of the central singularity is that of a corner. The radiation emitted very far from the black hole is thermal with temperature M/(2\pi). The back-reaction problem is solved to one-loop order.

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