Abstract
We give a new construction of conserved charges in asymptotically anti-de Sitter spacetimes in Einstein’s gravity. The new formula is explicitly gauge-invariant and makes direct use of the linearized curvature tensor instead of the metric perturbation. As an example, we compute the mass and angular momentum of the Kerr-AdS black holes.
- Received 2 November 2018
DOI:https://doi.org/10.1103/PhysRevD.99.044026
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Published by the American Physical Society
Physics Subject Headings (PhySH)
Gravitation, Cosmology & Astrophysics
