Vector Fields and Kerr/CFT Correspondence

  • Amir M. GhezelbashEmail author
Part of the Springer Proceedings in Physics book series (SPPHY, volume 170)


We use the appropriate boundary action for the vector fields near the horizon of near extremal Kerr black hole to calculate the two-point function for the vector fields in Kerr/CFT correspondence. The gauge-independent part of the two-point function is in agreement with what is expected from CFT.


Black Hole Kerr Black Hole Boundary Action Maxwell Field Kerr Spacetime 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.



This work was supported by the Natural Sciences and Engineering Research Council of Canada.


  1. 1.
    J.E. McClintock, R. Shafee, R. Narayan, R.A. Remillard, S.W. Davis, L.-X. Li, Astrophys. J. 652, 518 (2006)CrossRefADSGoogle Scholar
  2. 2.
    A. Castro, A. Maloney, A. Strominger, Phys. Rev. D 82, 024008 (2010)MathSciNetCrossRefADSGoogle Scholar
  3. 3.
    A.M. Ghezelbash, H.M. Siahaan, Class. Quantum Grav. 30, 135005 (2013)MathSciNetCrossRefADSGoogle Scholar
  4. 4.
    M. Becker, W. Schulgin, JHEP 1204, 063 (2012)MathSciNetCrossRefADSGoogle Scholar
  5. 5.
    T. Hartman, W. Song, A. Strominger, JHEP 1003, 118 (2010)CrossRefADSGoogle Scholar
  6. 6.
    A.M. Ghezelbashm, H.M. Siahaan, arXiv:1308.0096,
  7. 7.
    D.T. Son, A.O. Starinets, JHEP 0209, 042 (2002)MathSciNetCrossRefADSGoogle Scholar
  8. 8.
    B. Chen, C.-S. Chu, JHEP 1005, 004 (2010)MathSciNetCrossRefADSGoogle Scholar
  9. 9.
    I. Bredberg, T. Hartman, W. Song, A. Strominger, JHEP 1004, 019 (2010)MathSciNetCrossRefADSGoogle Scholar

Copyright information

© Springer International Publishing Switzerland 2016

Authors and Affiliations

  1. 1.Department of Physics and Engineering PhysicsUniversity of SaskatchewanSaskatoonCanada

Personalised recommendations