arXiv · 1810.13210
New thermodynamic identities for five-dimensional black holes
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Hari K. Kunduri, James Lucietti. 2019-03-13. New thermodynamic identities for five-dimensional black holes. https://doi.org/10.1088/1361-6382%2Fab0982
Cite the original work for its findings. Save a collection to share your selection of sources.