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Asymptotic expansions of the Cotton–York tensor on slices of stationary spacetimes

Juan Antonio Valiente Kroon

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We discuss expansions for the Cotton–York tensor near infinity for arbitrary slices of stationary spacetimes. From these expansions, it follows directly that a necessary condition for the existence of conformally flat slices in stationary solutions is the vanishing of a certain quantity of quadrupolar nature (obstruction). The obstruction is non-zero for the Kerr solution. Thus, the Kerr metric admits no conformally flat slices. An analysis of the next order terms in the expansions in the case of solutions such that the obstruction vanishes, suggests that the only stationary solutions admitting conformally flat slices are the Schwarzschild family of solutions.


PACS

04.20.-q Classical general relativity

04.25.D- Numerical relativity

02.30.Mv Approximations and expansions

MSC

41A60 Asymptotic approximations, asymptotic expansions (steepest descent, etc.) (See also 30E15)

83Cxx General relativity

Subjects

Mathematical physics

Gravitation and cosmology

Dates

Issue 13 (7 July 2004)

Received 5 February 2004

Published 8 June 2004



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