Annotation
In this paper we show that an isolated Kerr black hole can be interpreted as arising from a pair of identical counter-rotating NUT objects placed on a symmetry axis at the appropriate critical distance from each other.
Received: 2008 December 25
Approved: 2009 September 23
PACS:
04.20.Jb Exact solutions
04.70.Bw Classical black holes
97.60.Lf Black holes
04.70.Bw Classical black holes
97.60.Lf Black holes
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Authors
V.S. Manko$^1$, E.D. Rodchenko$^2$, E. Ruiz$^3$, M.B. Sadovnikova$^2$
$^1$Departamento de Física, Centro de Investigaçion y de Estudios Avanzados del IPN, A.P. 14-740, 07000, México D.F., Mexico
$^2$Department of Quantum Statistics and Field Theory, Moscow State University, Moscow, 119991, Russia
$^3$Instituto Universitario de Física Fundamental y Matemáticas, Universidad de Salamanca, 37008, Salamanca, Spain
$^1$Departamento de Física, Centro de Investigaçion y de Estudios Avanzados del IPN, A.P. 14-740, 07000, México D.F., Mexico
$^2$Department of Quantum Statistics and Field Theory, Moscow State University, Moscow, 119991, Russia
$^3$Instituto Universitario de Física Fundamental y Matemáticas, Universidad de Salamanca, 37008, Salamanca, Spain
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