Please use this identifier to cite or link to this item: https://doi.org/10.1103/PhysRevD.78.064062
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dc.titleRotating black lens solution in five dimensions
dc.contributor.authorChen, Y.
dc.contributor.authorTeo, E.
dc.date.accessioned2014-10-16T09:40:02Z
dc.date.available2014-10-16T09:40:02Z
dc.date.issued2008-09-23
dc.identifier.citationChen, Y., Teo, E. (2008-09-23). Rotating black lens solution in five dimensions. Physical Review D - Particles, Fields, Gravitation and Cosmology 78 (6) : -. ScholarBank@NUS Repository. https://doi.org/10.1103/PhysRevD.78.064062
dc.identifier.issn15507998
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/97847
dc.description.abstractIt has recently been shown that a stationary, asymptotically flat vacuum black hole in five space-time dimensions with two commuting axial symmetries must have an event horizon with either a spherical, ring or lens-space topology. In this paper, we study the third possibility, a so-called black lens with L(n,1) horizon topology. Using the inverse scattering method, we construct a black-lens solution with the simplest possible rod structure, and possessing a single asymptotic angular momentum. Its properties are then analyzed; in particular, it is shown that there must either be a conical singularity or a naked curvature singularity present in the space-time. © 2008 The American Physical Society.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1103/PhysRevD.78.064062
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentPHYSICS
dc.description.doi10.1103/PhysRevD.78.064062
dc.description.sourcetitlePhysical Review D - Particles, Fields, Gravitation and Cosmology
dc.description.volume78
dc.description.issue6
dc.description.page-
dc.description.codenPRVDA
dc.identifier.isiut000259692800133
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