Remarks on the Myers-Perry and Einstein-Gauss Rotating Solutions

A. Anabalón N. Deruelle 1 D. Tempo R. Troncoso
1 APC - THEORIE
Institut für theoretische Physik, APC - UMR 7164 - AstroParticule et Cosmologie
Abstract : The Kerr-type solutions of the five-dimensional Einstein and Einstein-Gauss-Bonnet equations look pretty similar when written in Kerr-Schild form. However the Myers-Perry spacetime is circular whereas the rotating solution of the Einstein-Gauss-Bonnet theory is not. We explore some consequences of this difference in particular regarding the (non)existence of Boyer-Lindquist-type coordinates and the extension of the manifold.
Type de document :
Article dans une revue
International Journal of Modern Physics D, World Scientific Publishing, 2011, 20, pp.639-647. <10.1142/S0218271811018974>


https://hal.archives-ouvertes.fr/hal-00740750
Contributeur : Alina Deniau <>
Soumis le : mercredi 10 octobre 2012 - 18:23:23
Dernière modification le : mardi 11 octobre 2016 - 14:55:48

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A. Anabalón, N. Deruelle, D. Tempo, R. Troncoso. Remarks on the Myers-Perry and Einstein-Gauss Rotating Solutions. International Journal of Modern Physics D, World Scientific Publishing, 2011, 20, pp.639-647. <10.1142/S0218271811018974>. <hal-00740750>

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