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      Bulk vs. Boundary Dynamics in Anti-de Sitter Spacetime

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          Abstract

          We investigate the details of the bulk-boundary correspondence in Lorentzian signature anti-de Sitter space. Operators in the boundary theory couple to sources identified with the boundary values of non-normalizable bulk modes. Such modes do not fluctuate and provide classical backgrounds on which bulk excitations propagate. Normalizable modes in the bulk arise as a set of saddlepoints of the action for a fixed boundary condition. They fluctuate and describe the Hilbert space of physical states. We provide an explicit, complete set of both types of modes for free scalar fields in global and Poincar\'e coordinates. For \ads3, the normalizable and non-normalizable modes originate in the possible representations of the isometry group \SLL×\SLR for a field of given mass. We discuss the group properties of mode solutions in both global and Poincar\'e coordinates and their relation to different expansions of operators on the cylinder and on the plane. Finally, we discuss the extent to which the boundary theory is a useful description of the bulk spacetime.

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          Stability in gauged extended supergravity

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            Gauge Theory Correlators from Non-Critical String Theory

            We suggest a means of obtaining certain Green's functions in 3+1-dimensional N=4 supersymmetric Yang-Mills theory with a large number of colors via non-critical string theory. The non-critical string theory is related to critical string theory in anti-deSitter background. We introduce a boundary of the anti-deSitter space analogous to a cut-off on the Liouville coordinate of the two-dimensional string theory. Correlation functions of operators in the gauge theory are related to the dependence of the supergravity action on the boundary conditions. From the quadratic terms in supergravity we read off the anomalous dimensions. For operators that couple to massless string states it has been established through absorption calculations that the anomalous dimensions vanish, and we rederive this result. The operators that couple to massive string states at level n acquire anomalous dimensions that grow as 2\left (n g_{YM} \sqrt {2 N} )^{1/2} for large `t Hooft coupling. This is a new prediction about the strong coupling behavior of large N SYM theory.
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              The Black Hole in Three Dimensional Space Time

              The standard Einstein-Maxwell equations in 2+1 spacetime dimensions, with a negative cosmological constant, admit a black hole solution. The 2+1 black hole -characterized by mass, angular momentum and charge, defined by flux integrals at infinity- is quite similar to its 3+1 counterpart. Anti-de Sitter space appears as a negative energy state separated by a mass gap from the continuous black hole spectrum. Evaluation of the partition function yields that the entropy is equal to twice the perimeter length of the horizon.
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                Author and article information

                Journal
                1998-05-26
                1998-07-27
                Article
                10.1103/PhysRevD.59.046003
                hep-th/9805171
                9d03efdb-e76b-40ab-b6bd-727b46d00bf0
                History
                Custom metadata
                Phys.Rev. D59 (1999) 046003
                Standard LaTeX, 28 pages, 2 postscript figures. v2: References added. Substantial revision in section 3 of treatment of global modes; non-normalizable modes have arbitrary time dependence. Revised discussion of low-mass modes and puzzle raised re: coupling of the dual boundary operators. v3: unwanted paragraph removed. v4: Sec. 5.2 corrected
                hep-th gr-qc

                General relativity & Quantum cosmology,High energy & Particle physics
                General relativity & Quantum cosmology, High energy & Particle physics

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