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Motion of charged particles around a five-dimensional rotating magnetized black hole

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dc.contributor.authorKaya, R.
dc.date.accessioned2026-06-27T13:04:42Z
dc.date.issued2007
dc.description.abstractWe study the effect of an external magnetic field on the stability of circular motion of charged particles in the equatorial plane of a five-dimensional rotating black hole. Using the Hamilton-Jacobi formalism, we derive the effective potential for the radial motion of test particles around a five-dimensional magnetized Myers-Perry black hole. We show that there exist stable circular orbits in equatorial planes in the background of this metric.en
dc.description.urihttps://doi.org/10.1142/s0218271807010663
dc.identifier.doi10.1142/s0218271807010663
dc.identifier.eissn1793-6594
dc.identifier.endpage1379
dc.identifier.issn0218-2718
dc.identifier.issue8
dc.identifier.startpage1369
dc.identifier.urihttps://hdl.handle.net/20.500.14981/49393
dc.identifier.volume16
dc.identifier.wos000252849300010
dc.language.isoeng
dc.publisherWORLD SCIENTIFIC PUBL CO PTE LTD
dc.relation.ispartofINTERNATIONAL JOURNAL OF MODERN PHYSICS D
dc.subjectgravity in more than four dimensions
dc.subjectclassical black holes
dc.subjectFIELD
dc.subjectEQUATIONS
dc.subjectENERGY
dc.subjectAstronomy & Astrophysics
dc.titleMotion of charged particles around a five-dimensional rotating magnetized black hole
dc.typeArticle
dspace.entity.typePublication
local.import.sourceWOS

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