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.
A new approach to conserved charges of generic gravity in AdS
Asymptotically anti-de Sitter spacetimes in topologically massive gravity
Comparison between various notions of conserved charges in asymptotically AdS-spacetimes
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