2005/02/15 by Nathalie Deruelle, Deruelle, Nathalie
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #gr-qc
paper · pdf · doi:10.48550/arxiv.gr-qc/0502072
14th Workshop On General Relativity And Gravitation (JGRG 2004) 29 Nov - 3 Dec 2004, Kyoto, Japan
arxiv created 2005/02/15 · openalex publication_date 2005/02/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We briefly review how to compute the mass and angular momenta of rotating, asymptotically anti-de Sitter spacetimes in Einstein-Gauss-Bonnet theory of gravity using superpotentials derived from standard Noether identities. The calculations depend on the asymptotic form of the metrics only and hence take no account of the source of the curvature. When the source of curvature is a black hole, the results can be checked using the first law of black hole thermodynamics.