Please use this identifier to cite or link to this item:
http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5184
Full metadata record
DC Field | Value | Language |
---|---|---|
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 |
Appears in Collections: | JOURNAL ARTICLES |
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.