Schwarzschild Black Holes from Matrix Theory

dc.creatorBanks, T.
dc.creatorFischler, W.
dc.creatorKlebanov, I. R.
dc.creatorSusskind, L.
dc.date1997-09-12
dc.date1997-09-18
dc.date.accessioned2026-07-07T10:53:50Z
dc.date.available2026-07-07T10:53:50Z
dc.descriptionWe consider Matrix theory compactified on T^3 and show that it correctly describes the properties of Schwarzschild black holes in 7+1 dimensions, including the energy-entropy relation, the Hawking temperature and the physical size, up to numerical factors of order unity. The most economical description involves setting the cut-off N in the discretized light-cone quantization to be of order the black hole entropy. A crucial ingredient necessary for our work is the recently proposed equation of state for 3+1 dimensional SYM theory with 16 supercharges. We give detailed arguments for the range of validity of this equation following the methods of Horowitz and Polchinski.
dc.description9 pages, latex; minor typos corrected
dc.identifierhttps://arxiv.org/abs/hep-th/9709091
dc.identifierhttp://arxiv.org/abs/hep-th/9709091
dc.identifierPhys.Rev.Lett.80:226-229,1998
dc.identifierdoi:10.1103/PhysRevLett.80.226
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185614
dc.subjectHigh Energy Physics - Theory
dc.titleSchwarzschild Black Holes from Matrix Theory
dc.typetext

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