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On fitting rotating bodies to exterior gravitational fields

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Abstract

Some inequalities have to be satisfied if there is to exist a fluid source for a given exterior gravitational field. In the case of the Kerr solution one of the inequalities presented here is much more restrictive than those obtained by Boyer [1]. However, our conditions do not exclude the possibility of a fluid source for the Kerr spacetimes.

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Communicated by J. Ehlers

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Abramowicz, M.A., Lasota, J.P. & Muchotrzeb, B. On fitting rotating bodies to exterior gravitational fields. Commun.Math. Phys. 47, 109–115 (1976). https://doi.org/10.1007/BF01608369

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  • DOI: https://doi.org/10.1007/BF01608369

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