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arXiv · hep-th/9712236

Evaporation of Schwarzschild Black Holes in Matrix Theory

T. Banks·W. Fischler·I. R. Klebanov
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Abstract

Recently, in collaboration with Susskind, we proposed a model of Schwarzschild black holes in Matrix theory. A large Schwarzschild black hole is described by a metastable bound state of a large number of D0-branes which are held together by a background, whose structure has so far been understood only in 8 and 11 dimensions. The Hawking radiation proceeds by emission of small clusters of D0-branes. We estimate the Hawking rate in the Matrix theory model of Schwarzschild black holes and find agreement with the semiclassical rate up to an undetermined numerical coefficient of order 1.

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T. Banks, W. Fischler, I. R. Klebanov. 1997-12-26. Evaporation of Schwarzschild Black Holes in Matrix Theory. https://doi.org/10.1016/s0370-2693(98)00118-x

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