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Phys. Rev. Lett. 80, 226–229 (1998)

Schwarzschild Black Holes from Matrix Theory

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T. Banks1, W. Fischler2, I. R. Klebanov3, and L. Susskind4,*
1Serin Physics Labs, Rutgers University, Piscataway, New Jersey 08855
2Physics Department, University of Texas, Austin, Texas 78712
3Joseph Henry Laboratories, Princeton University, Princeton, New Jersey 08544
4Institute for Advanced Study, Princeton, New Jersey 08540

Received 22 September 1997; published in the issue dated 12 January 1998

We consider matrix theory compactified on T3 and show that it correctly describes the properties of Schwarzschild black holes in 7+1 dimensions, including the mass-entropy relation, the Hawking temperature, and the physical size, up to numerical factors of order unity. The most economical description involves setting the cutoff 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 supersymmetric Yang-Mills theory with 16 supercharges. We give detailed arguments for the range of validity of this equation following the methods of Horowitz and Polchinski.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.80.226
DOI:
10.1103/PhysRevLett.80.226
PACS:
04.70.Dy, 11.10.Kk, ll.25.Mj

*Permanent address: Physics Department, Stanford University, Stanford, CA 94305.