31
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: found
      • Article: found
      Is Open Access

      Spinning strings in AdS_5 x S^5: new integrable system relations

      Preprint
      , ,

      Read this article at

      ScienceOpenPublisherArXiv
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          A general class of rotating closed string solutions in AdS_5 x S^5 is shown to be described by a Neumann-Rosochatius one-dimensional integrable system. The latter represents an oscillator on a sphere or a hyperboloid with an additional ``centrifugal'' potential. We expect that the reduction of the AdS_5 x S^5 sigma model to the Neumann-Rosochatius system should have further generalizations and should be useful for uncovering new relations between integrable structures on the two sides of the AdS/CFT duality. We find, in particular, new circular rotating string solutions with two AdS_5 and three S^5 spins. As in other recently discussed examples, the leading large-spin correction to the classical energy turns out to be proportional to the square of the string tension or the 't Hooft coupling \lambda, suggesting that it can be matched onto the one-loop anomalous dimensions of the corresponding ``long'' operators on the SYM side of the AdS/CFT duality.

          Related collections

          Most cited references3

          • Record: found
          • Abstract: not found
          • Article: not found

          Exact integrability of strings inD-dimensional de Sitter spacetime

            • Record: found
            • Abstract: found
            • Article: found
            Is Open Access

            Planetoid String Solutions in 3 + 1 Axisymmetric Spacetimes

            The string propagation equations in axisymmetric spacetimes are exactly solved by quadratures for a planetoid Ansatz. This is a straight non-oscillating string, radially disposed, which rotates uniformly around the symmetry axis of the spacetime. In Schwarzschild black holes, the string stays outside the horizon pointing towards the origin. In de Sitter spacetime the planetoid rotates around its center. We quantize semiclassically these solutions and analyze the spin/(mass\(^2\)) (Regge) relation for the planetoids, which turns out to be non-linear.
              • Record: found
              • Abstract: not found
              • Article: not found

              Relativistic string model in a space-time of a constant curvature

                Author and article information

                Journal
                02 November 2003
                2004-11-23
                Article
                10.1103/PhysRevD.69.086009
                hep-th/0311004
                4a194937-f74e-4162-bd14-53453f5dca55
                History
                Custom metadata
                AEI-2003-091
                Phys.Rev.D69:086009,2004
                Latex, 33 pages; v2: few minor misprints corrected
                hep-th

                Comments

                Comment on this article

                Related Documents Log