Abstract
We compute the mass, angular momenta, and charge of the Gödel-type rotating black hole solution to five-dimensional minimal supergravity. A generalized Smarr formula is derived, and the first law of thermodynamics is verified. The computation rests on a new approach to conserved charges in gauge theories that allows for their computation at finite radius.
- Received 25 January 2005
DOI:https://doi.org/10.1103/PhysRevLett.95.031302
©2005 American Physical Society