Slowly varying dilaton cosmologies and their field theory duals

Adel Awad, Sumit R. Das, Archisman Ghosh, Jae-Hyuk Oh, and Sandip P. Trivedi
Phys. Rev. D 80, 126011 – Published 18 December 2009

Abstract

We consider a deformation of the AdS5×S5 solution of IIB supergravity obtained by taking the boundary value of the dilaton to be time dependent. The time dependence is taken to be slowly varying on the anti-de Sitter (AdS) scale thereby introducing a small parameter ϵ. The boundary dilaton has a profile which asymptotes to a constant in the far past and future and attains a minimum value at intermediate times. We construct the supergravity (sugra) solution to first nontrivial order in ϵ, and find that it is smooth, horizon-free, and asymptotically AdS5×S5 in the far future. When the intermediate values of the dilaton becomes small enough the curvature becomes of order the string scale and the sugra approximation breaks down. The resulting dynamics is analyzed in the dual SU(N) gauge theory on S3 with a time dependent coupling constant which varies slowly. When Nϵ1, we find that a quantum adiabatic approximation is applicable, and use it to argue that at late times the geometry becomes smooth AdS5×S5 again. When Nϵ1, we formulate a classical adiabatic perturbation theory based on coherent states which arises in the large N limit. For large values of the ’t Hooft coupling this reproduces the supergravity results. For small ’t Hooft coupling the coherent state calculations become involved and we cannot reach a definite conclusion. We argue that the final state should have a dual description which is mostly smooth AdS5 space with the possible presence of a small black hole.

  • Received 24 August 2009

DOI:https://doi.org/10.1103/PhysRevD.80.126011

©2009 American Physical Society

Authors & Affiliations

Adel Awad1,2,*, Sumit R. Das3,†, Archisman Ghosh3,‡, Jae-Hyuk Oh3,§, and Sandip P. Trivedi4,5,6,∥

  • 1Center for Theoretical Physics, British University of Egypt, Sherouk City 11837, P.O. Box 43, EGYPT
  • 2Department of Physics, Faculty of Science, Ain Shams University, Cairo, 11566, EGYPT
  • 3Department of Physics and Astronomy, University of Kentucky, Lexington, Kentucky 40506, USA
  • 4Tata Institute of Fundamental Research, Mumbai 400005, India
  • 5Stanford Institute of Theoretical Physics, Stanford, California 94305, USA
  • 6SLAC, Stanford University, Stanford, California 94309, USA

  • *adel@pa.uky.edu
  • das@pa.uky.edu
  • archisman.ghosh@uky.edu
  • §jaehyukoh@uky.edu
  • trivedi.sp@gmail.com

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Issue

Vol. 80, Iss. 12 — 15 December 2009

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