Counterrotating perfect fluid discs as sources of electrovacuum static spacetimes

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dc.creatorGarcía-Reyes, Gonzalo
dc.creatorGonzález, Guillermo A.
dc.date2008-10-14
dc.date.accessioned2026-07-07T12:15:50Z
dc.date.available2026-07-07T12:15:50Z
dc.descriptionThe interpretation of some electrovacuum spacetimes in terms of counterrotating perfect fluid discs is presented. The interpretation is mades by means of an "inverse problem" approach used to obtain disc sources of known static solutions of the Einstein-Maxwell equations. In order to do such interpretation, a detailed study is presented of the counterrotating model (CRM) for generic electrovacuum static axially symmetric relativistic thin discs with nonzero radial pressure. Four simple families of models of counterrotating charged discs based on Chazy-Curzon-type, Zipoy-Voorhees-type, Bonnor-Sackfield-type, and charged and magnetized Darmois electrovacuum metrics are considered where we obtain some discs with a CRM well behaved.
dc.description22 pages, 4 figures, LaTeX2e
dc.identifierhttps://arxiv.org/abs/0810.2567
dc.identifierhttp://arxiv.org/abs/0810.2567
dc.identifierClass.Quant.Grav.21:4845-4864,2004
dc.identifierdoi:10.1088/0264-9381/21/21/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211610
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCounterrotating perfect fluid discs as sources of electrovacuum static spacetimes
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