Abstract
We construct the perturbative solution of the charged black hole in the Kaluza-Klein spacetime with the matched asymptotic expansion method. The corrections to the thermodynamic variables are calculated up to the post-Newtonian order. We confirmed that the method can work very well in the Einstein-Maxwell theory.
- Received 25 May 2012
DOI:https://doi.org/10.1103/PhysRevD.86.044018
© 2012 American Physical Society
