Geodesic motion in the (rotating) black string spacetime

dc.contributor.author	Grunau, Saskia	en_US
dc.contributor.author	KHAMESRA, BHAVESH	en_US
dc.date.accessioned	2020-10-19T08:59:38Z
dc.date.available	2020-10-19T08:59:38Z
dc.date.issued	2013-06	en_US
dc.identifier.citation	Physical Review D, 87(12).	en_US
dc.identifier.issn	2470-0029	en_US
dc.identifier.issn	2470-0010	en_US
dc.identifier.uri	http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5184
dc.identifier.uri	https://doi.org/10.1103/PhysRevD.87.124019	en_US
dc.description.abstract	In 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 spacetime	en_US
dc.language.iso	en	en_US
dc.publisher	American Physical Society	en_US
dc.subject	Physics	en_US
dc.subject	2013	en_US
dc.title	Geodesic motion in the (rotating) black string spacetime	en_US
dc.type	Article	en_US
dc.contributor.department	Dept. of Physics	en_US
dc.identifier.sourcetitle	Physical Review D	en_US
dc.publication.originofpublisher	Foreign	en_US