Geodesic motion in the (rotating) black string spacetime

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dc.contributor.authorGrunau, Saskiaen_US
dc.contributor.authorKHAMESRA, BHAVESHen_US
dc.contributor.departmentDept. of Physicsen_US
dc.date.accessioned2020-10-19T08:59:38Z
dc.date.available2020-10-19T08:59:38Z
dc.date.issued2013-06en_US
dc.description.abstractIn this article we study the geodesic motion of test particles and light in the five-dimensional (rotating) black string spacetime. If a compact dimension is added to the four-dimensional Schwarzschild or Kerr spacetime, the new five-dimensional metric describes a (rotating) black string. The geodesics in the Schwarzschild and Kerr spacetime have been studied in great detail; however, when a compact dimension is added new behavior occurs. We present the analytical solutions of the geodesic equations and discuss the possible orbits. The motion in the ordinary four-dimensional Schwarzschild and Kerr spacetime is compared to the motion in the (rotating) black string spacetimeen_US
dc.identifier.citationPhysical Review D, 87(12).en_US
dc.identifier.issn2470-0029en_US
dc.identifier.issn2470-0010en_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5184
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.87.124019
dc.language.isoenen_US
dc.publication.originofpublisherForeignen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectPhysicsen_US
dc.subject2013en_US
dc.titleGeodesic motion in the (rotating) black string spacetimeen_US
dc.typeArticleen_US

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