1997/05/19 by F. Vendrell, Vendrell, F. · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Relativity and Gravitational Theory #gr-qc #hep-th
paper · pdf · doi:10.48550/arxiv.hep-th/9705135
12 pages, Revtex, 2 figures
arxiv created 1997/05/19 · arxiv updated 2009/11/30
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/(2π). The back-reaction problem is solved to one-loop order.