Caged black hole with Maxwell charge

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.

17 pages

References in corpus (5)

• Instabilities of Black Strings and Branes
• Classical Effective Field Theory and Caged Black Holes
• Asymptotics of d-dimensional Kaluza-Klein black holes: beyond the Newtonian approximation
• Harrison transformation and charged black objects in Kaluza-Klein theory
• Higher dimensional black holes

Cited by in corpus (2)

• Lumpy AdS${}_5\times$ S${}^5$ Black Holes and Black Belts
• Stable circular orbits in caged black hole spacetimes