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

By A. Anabalón, N. Deruelle, D. Tempo and R. Troncoso


International audienceThe 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

Topics: Myers-Perry, Einstein-Gauss-Bonnet, rotating solutions, [ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], [ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]
Publisher: World Scientific Publishing
Year: 2011
DOI identifier: 10.1142/S0218271811018974
OAI identifier: oai:HAL:hal-00740750v1
Provided by: Hal-Diderot
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