J B Griffiths and J Podolský 2007 Class. Quantum Grav. 24 1687 doi:10.1088/0264-9381/24/6/N02
J B Griffiths1 and J Podolský2
Show affiliationsDifferent forms of the metric for the Kerr–NUT–(anti-)de Sitter spacetime are being widely used in its extension to higher dimensions. The purpose of this note is to relate the parameters that are being used to the physical parameters (mass, rotation, NUT and cosmological constant) in the basic four-dimensional situation.
04.70.-s Physics of black holes
Issue 6 (21 March 2007)
Received 26 January 2007
Published 6 March 2007
J B Griffiths and J Podolský 2007 Class. Quantum Grav. 24 1687
Jérôme Martin et al JHEP03(2005)060
Huang She-Song et al 2008 Chinese Phys. B 17 323
Vl.V. Bobkov et al 2006 Nucl. Fusion 46 S469
Cheng Rong Li and Tsin Chi Yang 1991 J. Phys. D: Appl. Phys. 24 48
J A Blanco and J Pisonero 1999 Eur. J. Phys. 20 289
Andrés Mujica and R J Needs 1996 J. Phys.: Condens. Matter 8 L237
Richard H Bayford and Alex Hartov 2009 Physiol. Meas. 30
Kurt Bryan and Lester Caudill 2005 Inverse Problems 21 239
Myrlene Gee and Stuart G Whittington 1997 J. Phys. A: Math. Gen. 30 L1