Black holes and the SYM phase diagram. II

Journal Article · Tue Jun 01 00:00:00 EDT 1999 · Physical Review, D

DOI:https://doi.org/10.1103/PhysRevD.59.124005· OSTI ID:341450

Martinec, E; Sahakian, V ^[1]

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1. Enrico Fermi Institute and Department of Physics, University of Chicago, 5640 S. Ellis Avenue, Chicago, Illinois 60637 (United States)

The complete phase diagram of objects in M theory compactified on tori T{sup p},p=1,2,3, is elaborated. Phase transitions occur when the object localizes on cycle(s) (the Gregory-Laflamme transition), or when the area of the localized part of the horizon becomes one in string units (the Horowitz-Polchinski correspondence point). The low-energy, near-horizon geometry that governs a given phase can match onto a variety of asymptotic regimes. The analysis makes it clear that the matrix conjecture is a special case of the Maldacena conjecture. {copyright} {ital 1999} {ital The American Physical Society}

• OSTI ID: 341450
• Journal Information: Physical Review, D, Vol. 59, Issue 12; Other Information: PBD: Jun 1999
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
UNIFIED GAUGE MODELS
PHASE DIAGRAMS
UNIFIED-FIELD THEORIES
SUPERSYMMETRY
YANG-MILLS THEORY
BLACK HOLES
THERMODYNAMICS