Vector Fields and Kerr/CFT Correspondence
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.
KeywordsBlack Hole Kerr Black Hole Boundary Action Maxwell Field Kerr Spacetime
This work was supported by the Natural Sciences and Engineering Research Council of Canada.