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arXiv · 1009.3030

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

A. Anabalon·N. Deruelle·D. Tempo·R. Troncoso
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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.

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A. Anabalon, N. Deruelle, D. Tempo, R. Troncoso. 2010-09-15. Remarks on the Myers-Perry and Einstein Gauss-Bonnet Rotating Solutions. https://doi.org/10.1142/s0218271811018974

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