Entropy and temperature of black 3-branes

S. S. Gubser, I. R. Klebanov, A. W. Peet

Research output: Contribution to journalArticlepeer-review

431 Scopus citations

Abstract

We consider slightly nonextremal black 3-branes of type IIB supergravity and show that their Bekenstein-Hawking entropy agrees, up to a mysterious factor, with an entropy derived by counting non-BPS excitations of the Dirichlet 3-brane. These excitations are described in terms of the statistical mechanics of a (3+1)-dimensional gas of massless open string states. This is essentially the classic problem of blackbody radiation. The blackbody temperature is related to the temperature of the Hawking radiation. We also construct a solution of type IIB supergravity describing a 3-brane with a finite density of longitudinal momentum. For extremal momentum-carrying 3-branes the horizon area vanishes. This is in agreement with the fact that the BPS entropy of the momentum-carrying Dirichlet 3-branes is not an extensive quantity.

Original languageEnglish (US)
Pages (from-to)3915-3919
Number of pages5
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume54
Issue number6
DOIs
StatePublished - 1996

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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