January 1992, DSF-92/6 SINGULARITY THEORY IN CLASSICAL COSMOLOGY
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چکیده
منابع مشابه
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The formation and semi-classical evaporation of two-dimensional black holes is studied in an exactly solvable model. Above a certain threshold energy flux, collapsing matter forms a singularity inside an apparent horizon. As the black hole evaporates the apparent horizon recedes and meets the singularity in a finite proper time. The singularity emerges naked and future evolution of the geometry...
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