Harrison transformation and charged black objects in Kaluza-Klein theory
Burkhard Kleihaus, Jutta Kunz, Eugen Radu, Cristian Stelea

TL;DR
This paper constructs charged black brane solutions in higher-dimensional Kaluza-Klein theory using Harrison transformations, analyzes their thermodynamics, and explores stability and topology-changing transitions, including spinning solutions with nontrivial gyromagnetic ratios.
Contribution
It introduces a method to generate charged black objects in Kaluza-Klein theory via Harrison transformations and extends the quasilocal formalism to compute their charges.
Findings
Charged solutions are thermodynamically unstable in grand canonical ensemble.
Topology-changing transitions are consistent with previous vacuum case scenarios.
Spinning solutions exhibit a gyromagnetic ratio dependent on nonuniformity.
Abstract
We generate charged black brane solutions in dimensions in a theory of gravity coupled to a dilaton and an antisymmetric form, by using a Harrison-type transformation. The seed vacuum solutions that we use correspond to uplifted Kaluza-Klein black strings and black holes in -dimensions. A generalization of the Marolf-Mann quasilocal formalism to the Kaluza-Klein theory is also presented, the global charges of the black objects being computed in this way. We argue that the thermodynamics of the charged solutions can be derived from that of the vacuum configurations. Our results show that all charged Kaluza-Klein solutions constructed by means of Harrison transformations are thermodynamically unstable in a grand canonical ensemble. The general formalism is applied to the case of nonuniform black strings and caged black hole solutions in Einstein-Maxwell-dilaton…
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