New thermodynamic identities for five-dimensional black holes
arXiv:1810.13210 · doi:10.1088/1361-6382/ab0982
Abstract
We derive new identities for the thermodynamic variables of five-dimensional, asymptotically flat, stationary and biaxisymmetric vacuum black holes. These identities depend on the topology of the solution and include contributions arising from certain topological charges. The proof employs the harmonic map formulation of the vacuum Einstein equations for solutions with these symmetries.
5 pages. v2: minor edits
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