Abstract
In this paper, we use the appropriate boundary action for the vector fields near the horizon of the near extremal Kerr black hole to calculate the two-point function for the vector fields in Kerr/CFT correspondence. We show the gauge-independent part of the two-point function is in agreement with what is expected from CFT.
- Received 16 October 2013
DOI:https://doi.org/10.1103/PhysRevD.89.024017
© 2014 American Physical Society
