Nathalie Deruelle and Joseph Katz 2005 Class. Quantum Grav. 22 421 doi:10.1088/0264-9381/22/2/013
Nathalie Deruelle1,2 and Joseph Katz3,4
Show affiliationsWe show how to compute the mass of a Kerr–anti-de Sitter spacetime with respect to the anti-de Sitter background in any dimension, using a superpotential which has been derived from standard Noether identities. The calculation takes no account of the source of the curvature and confirms results obtained for black holes via the first law of thermodynamics.
04.70.-s Physics of black holes
04.50.-h Higher-dimensional gravity and other theories of gravity
Issue 2 (21 January 2005)
Received 28 October 2004
Published 3 January 2005
Nathalie Deruelle and Joseph Katz 2005 Class. Quantum Grav. 22 421
Philip Ball 2002 Nanotechnology 13 R15
M M Akbar and Saurya Das 2004 Class. Quantum Grav. 21 1383
John W Norbury 1989 Eur. J. Phys. 10 237
H Henriksson et al 2002 Plasma Phys. Control. Fusion 44 1253
G. Giruzzi et al 1997 Nucl. Fusion 37 673
M R Smith and D G Hughes 1971 J. Phys. E: Sci. Instrum. 4 725
R L Rusby and C A Swenson 1980 Metrologia 16 73
B R Judd 1987 J. Phys. A: Math. Gen. 20 L343
S Myneni et al 2002 J. Phys.: Condens. Matter 14 L213