Remarks on the myers-perry and Einstein-Gauss-Bonnet rotating solutions

Andres Anabalón; Nathalie Deruelle; David Tempo; Ricardo Troncoso

doi:10.1142/S0218271811018974

Remarks on the myers-perry and Einstein-Gauss-Bonnet rotating solutions

Andres Anabalón^*, Nathalie Deruelle, David Tempo, Ricardo Troncoso

^*Autor correspondiente de este trabajo

Producción científica: Contribución a una revista › Artículo › revisión exhaustiva

19 Citas (Scopus)

Resumen

The Kerr-type solutions of the five-dimensional Einstein and Einstein-Gauss-Bonnet equations look pretty similar when written in KerrSchild 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 BoyerLindquist-type coordinates and the extension of the manifold.

Idioma original	Inglés
Páginas (desde-hasta)	639-647
Número de páginas	9
Publicación	International Journal of Modern Physics D
Volumen	20
N.º	5
DOI	https://doi.org/10.1142/S0218271811018974
Estado	Publicada - 2011
Publicado de forma externa	Sí

Áreas temáticas de ASJC Scopus

Física matemática
Astronomía y astrofísica
Ciencias planetarias y espacial

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title = "Remarks on the myers-perry and Einstein-Gauss-Bonnet rotating solutions",

abstract = "The Kerr-type solutions of the five-dimensional Einstein and Einstein-Gauss-Bonnet equations look pretty similar when written in KerrSchild 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 BoyerLindquist-type coordinates and the extension of the manifold.",

keywords = "Einstein-Gauss-Bonnet, Myers-Perry, rotating solutions",

author = "Andres Anabal{\'o}n and Nathalie Deruelle and David Tempo and Ricardo Troncoso",

note = "Funding Information: This research is partially funded by FONDECYT grants Nos. 1085322, 1095098, 3110141, and by the Conicyt grant ACT-91: “Southern Theoretical Physics Laboratory” (STPLab). The Centro de Estudios Cient{\'i}ficos (CECS) is funded by the Chilean Government through the Centers of Excellence Base Financing Program of Conicyt. CIN is funded by Conicyt and the Gobierno Regional de Los R{\'i}os.",

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AU - Anabalón, Andres

AU - Deruelle, Nathalie

AU - Tempo, David

AU - Troncoso, Ricardo

N1 - Funding Information: This research is partially funded by FONDECYT grants Nos. 1085322, 1095098, 3110141, and by the Conicyt grant ACT-91: “Southern Theoretical Physics Laboratory” (STPLab). The Centro de Estudios Científicos (CECS) is funded by the Chilean Government through the Centers of Excellence Base Financing Program of Conicyt. CIN is funded by Conicyt and the Gobierno Regional de Los Ríos.

PY - 2011/5/20

Y1 - 2011/5/20

N2 - The Kerr-type solutions of the five-dimensional Einstein and Einstein-Gauss-Bonnet equations look pretty similar when written in KerrSchild 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 BoyerLindquist-type coordinates and the extension of the manifold.

AB - The Kerr-type solutions of the five-dimensional Einstein and Einstein-Gauss-Bonnet equations look pretty similar when written in KerrSchild 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 BoyerLindquist-type coordinates and the extension of the manifold.

KW - Einstein-Gauss-Bonnet

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Remarks on the myers-perry and Einstein-Gauss-Bonnet rotating solutions

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