Rotating solutions in critical Lovelock gravities

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 gravit...

Full description

Bibliographic Details
Main Authors: M. Cvetič, Xing-Hui Feng, H. Lü, C.N. Pope
Format: Article
Language:English
Published: Elsevier 2017-02-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316307560
id doaj-f3ac925c212348289b62782b36e48234
record_format Article
spelling doaj-f3ac925c212348289b62782b36e482342020-11-24T20:40:39ZengElsevierPhysics Letters B0370-26931873-24452017-02-01765C18118710.1016/j.physletb.2016.12.018Rotating solutions in critical Lovelock gravitiesM. Cvetič0Xing-Hui Feng1H. Lü2C.N. Pope3Department of Physics, Beijing Normal University, Beijing, 100875, ChinaDepartment of Physics, Beijing Normal University, Beijing, 100875, ChinaDepartment of Physics, Beijing Normal University, Beijing, 100875, ChinaDepartment of Physics, Beijing Normal University, Beijing, 100875, ChinaFor 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.http://www.sciencedirect.com/science/article/pii/S0370269316307560
collection DOAJ
language English
format Article
sources DOAJ
author M. Cvetič
Xing-Hui Feng
H. Lü
C.N. Pope
spellingShingle M. Cvetič
Xing-Hui Feng
H. Lü
C.N. Pope
Rotating solutions in critical Lovelock gravities
Physics Letters B
author_facet M. Cvetič
Xing-Hui Feng
H. Lü
C.N. Pope
author_sort M. Cvetič
title Rotating solutions in critical Lovelock gravities
title_short Rotating solutions in critical Lovelock gravities
title_full Rotating solutions in critical Lovelock gravities
title_fullStr Rotating solutions in critical Lovelock gravities
title_full_unstemmed Rotating solutions in critical Lovelock gravities
title_sort rotating solutions in critical lovelock gravities
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2017-02-01
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.
url http://www.sciencedirect.com/science/article/pii/S0370269316307560
work_keys_str_mv AT mcvetic rotatingsolutionsincriticallovelockgravities
AT xinghuifeng rotatingsolutionsincriticallovelockgravities
AT hlu rotatingsolutionsincriticallovelockgravities
AT cnpope rotatingsolutionsincriticallovelockgravities
_version_ 1716826114506096640