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      Blackhole/String Transition for the Small Schwarzschild Blackhole of AdS5×S5 and Critical Unitary Matrix Models

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          Abstract

          In this paper we discuss the blackhole-string transition of the small Schwarzschild blackhole of AdS5×S5 using the AdS/CFT correspondence at finite temperature. The finite temperature gauge theory effective action, at weak {\it and} strong coupling, can be expressed entirely in terms of constant Polyakov lines which are SU(N) matrices. In showing this we have taken into account that there are no Nambu-Goldstone modes associated with the fact that the 10 dimensional blackhole solution sits at a point in S5. We show that the phase of the gauge theory in which the eigenvalue spectrum has a gap corresponds to supergravity saddle points in the bulk theory. We identify the third order N= phase transition with the blackhole-string transition. This singularity can be resolved using a double scaling limit in the transition region where the large N expansion is organized in terms of powers of N2/3. The N= transition now becomes a smooth crossover in terms of a renormalized string coupling constant, reflecting the physics of large but finite N. Multiply wound Polyakov lines condense in the crossover region. We also discuss the implications of our results for the resolution of the singularity of the Lorenztian section of the small Schwarzschild blackhole.

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          The Hagedorn/Deconfinement Phase Transition in Weakly Coupled Large N Gauge Theories

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            A Correspondence Principle for Black Holes and Strings

            For most black holes in string theory, the Schwarzschild radius in string units decreases as the string coupling is reduced. We formulate a correspondence principle, which states that (i) when the size of the horizon drops below the size of a string, the typical black hole state becomes a typical state of strings and D-branes with the same charges, and (ii) the mass does not change abruptly during the transition. This provides a statistical interpretation of black hole entropy. This approach does not yield the numerical coefficient, but gives the correct dependence on mass and charge in a wide range of cases, including neutral black holes.
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              Extended particles in quantum field theories

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                Author and article information

                Journal
                03 May 2006
                2006-09-03
                Article
                10.1140/epjc/s10052-006-0049-x
                hep-th/0605041
                892dd93f-8ce8-4ec0-b77c-3d4374939f1a
                History
                Custom metadata
                CERN-PH-TH/2006-078, TIFR/TH/06-01
                Eur.Phys.J.C48:647-665,2006
                44 pages, Minor changes,the submitted version in the journal
                hep-th

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