Quantum back reaction to asymptotically AdS black holes

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Abstract

We analyze the effects of the back reaction due to a conformal field theory (CFT) on a black hole spacetime with negative cosmological constant. We study the geometry numerically obtained by taking into account the energy momentum tensor of CFT approximated by a radiation fluid. We find a sequence of configurations without a horizon in thermal equilibrium (CFT stars), followed by a sequence of configurations with a horizon. We discuss the thermodynamic properties of the system and how back reaction effects alter the space-time structure. We also provide an interpretation of the above sequence of solutions in terms of the AdS/CFT correspondence. The dual five-dimensional description is given by the Karch-Randall model, in which a sequence of five-dimensional floating black holes followed by a sequence of brane localized black holes correspond to the above solutions.

Journal

  • Journal of High Energy Physics

    Journal of High Energy Physics 2010(1), 1-24, 2010-01

    Springer Verlag

Codes

  • NII Article ID (NAID)
    120002462957
  • NII NACSIS-CAT ID (NCID)
    AA11380940
  • Text Lang
    ENG
  • Article Type
    journal article
  • ISSN
    1126-6708
  • Data Source
    IR 
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