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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://dk.um.si/IzpisGradiva.php?id=69868"><dc:title>Rotating solutions in critical Lovelock gravities</dc:title><dc:creator>Cvetič,	Mirjam	(Avtor)
	</dc:creator><dc:creator>Feng,	Xing-Hui	(Avtor)
	</dc:creator><dc:creator>Lü,	Hong	(Avtor)
	</dc:creator><dc:creator>Pope,	Christopher N.	(Avtor)
	</dc:creator><dc:subject>astrophysics</dc:subject><dc:subject>nuclear physics</dc:subject><dc:description>For appropriate choices of the coupling constants, the equations of motion of Lovelock gravities up to order n in the Riemann tensor can be factorized such that the theories admit a single (A)dS vacuum. In this paper we construct two classes of exact rotating metrics in such critical Lovelock gravities of order n in d = 2n +1 dimensions. In one class, the n angular momenta in the n orthogonal spatial 2-planes are equal, and hence the metric is of cohomogeneity one. We construct these metrics in a Kerr-Schild form, but they can then be recast in terms of Boyer-Lindquist coordinates. The other class involves metrics with only a single non-vanishing angular momentum. Again we construct them in a Kerr-Schild form, but in this case it does not seem to be possible to recast them in Boyer-Lindquist form. Both classes of solutions have naked curvature singularities, arising because of the over rotation of the configurations.</dc:description><dc:date>2017</dc:date><dc:date>2018-03-08 09:17:41</dc:date><dc:type>Znanstveno delo</dc:type><dc:identifier>69868</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
