dc.creatorGürlebeck N.
dc.creatorBičák J.
dc.creatorGutiérrez-Piñeres A.C.
dc.date.accessioned2020-03-26T16:32:58Z
dc.date.accessioned2022-09-28T20:12:15Z
dc.date.available2020-03-26T16:32:58Z
dc.date.available2022-09-28T20:12:15Z
dc.date.created2020-03-26T16:32:58Z
dc.date.issued2011
dc.identifierGeneral Relativity and Gravitation; Vol. 43, Núm. 12; pp. 3301-3312
dc.identifier00017701
dc.identifierhttps://hdl.handle.net/20.500.12585/9108
dc.identifier10.1007/s10714-011-1234-2
dc.identifierUniversidad Tecnológica de Bolívar
dc.identifierRepositorio UTB
dc.identifier24504208500
dc.identifier35562832600
dc.identifier25225467000
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3722505
dc.description.abstractIn the Introduction we briefly recall our previous results on stationary electromagnetic fields on black hole backgrounds and the use of spin-weighted spherical harmonics. We then discuss static electric and magnetic test fields in a Schwarzschild background using some of these results. As sources we do not consider point charges or current loops like in previous works, rather, we analyze spherical shells with smooth electric or magnetic charge distributions as well as electric or magnetic dipole distributions depending on both angular coordinates. Particular attention is paid to the discontinuities of the field, of the 4-potential, and their relation to the source. © 2011 Springer Science+Business Media, LLC.
dc.languageeng
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.rightsAtribución-NoComercial 4.0 Internacional
dc.sourcehttps://www.scopus.com/inward/record.uri?eid=2-s2.0-81555211144&doi=10.1007%2fs10714-011-1234-2&partnerID=40&md5=511538f1247c03df354be140d6cd38d3
dc.titleElectromagnetic sources distributed on shells in a Schwarzschild background


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