An infinite family of relativistic magnetized finite thin disks
An infinite family of relativistic finite thin disk model with magnetic field is presented. The model is obtained for solving the Einstein-Maxwell equations for static spacetimes by means of the Horsk-Mitskievitch generating conjecture. The vacuum limit of these obtained solutions is the well known...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2011
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/9114
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/9114
- Palabra clave:
- Magnetic fields
Maxwell equations
Einstein Maxwell equations
Energy condition
Energy-momentum tensor
Oblate spheroidal coordinates
Physical quantities
Thin disk
Relativity
- Rights
- restrictedAccess
- License
- http://creativecommons.org/licenses/by-nc-nd/4.0/
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2020-03-26T16:32:59Z2020-03-26T16:32:59Z2011Journal of Physics: Conference Series; Vol. 314, Núm. 117426588https://hdl.handle.net/20.500.12585/911410.1088/1742-6596/314/1/012090Universidad Tecnológica de BolívarRepositorio UTB543970500007202571265An infinite family of relativistic finite thin disk model with magnetic field is presented. The model is obtained for solving the Einstein-Maxwell equations for static spacetimes by means of the Horsk-Mitskievitch generating conjecture. The vacuum limit of these obtained solutions is the well known Morgan and Morgan solution. The obtained expressions are simply written in terms of oblate spheroidal coordinates. The mass of the disks are finite and the energy-momentum tensor agrees with all the energy conditions. The magnetic field and the circular velocity are evaluated explicitly. All the physical quantities obtained shown an acceptable behavior © Published under licence by IOP Publishing Ltd.Recurso electrónicoapplication/pdfengInstitute of Physics Publishinghttp://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/restrictedAccessAtribución-NoComercial 4.0 Internacionalhttp://purl.org/coar/access_right/c_16echttps://www.scopus.com/inward/record.uri?eid=2-s2.0-81455154977&doi=10.1088%2f1742-6596%2f314%2f1%2f012090&partnerID=40&md5=1766de214272a8963422289e2233df12Spanish Relativity Meeting: Gravity as a Crossroad in Physics, ERE 2010An infinite family of relativistic magnetized finite thin disksinfo:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionConferenciahttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_c94fMagnetic fieldsMaxwell equationsEinstein Maxwell equationsEnergy conditionEnergy-momentum tensorOblate spheroidal coordinatesPhysical quantitiesThin diskRelativityGranada6 September 2010 through 10 September 2010Gutiérrez-Piñeres A.C.González G.A.Lichnerowicz, A., R. C, (1971) Acad. Sci., 273, p. 528Taub, A.H., (1980) J. Math. Phys., 21 (6), p. 1423Gonzlez, G.A., Espitia, O.A., (2003) Phys. Rev. D, 68 (10), p. 104028García-Reyes, G., Gonzlez, G.A., (2004) Phys. Rev. D, 70 (10), p. 104005Richtereck, L., Novotn, J., Horsk, J., (2000) Czech. J. Phys., 50 (8), p. 925Morgan, T., Morgan, L., (1969) Phys. Rev., 183 (5), p. 1097Arfken, G., Weber, H., (2005) Mathematical Methods for Physicists, , Academic Press, New YorkMorse, P.M., Fesbach, H., (1953) Methods of Theoretical Physics, , McGraw-HillGonzlez, G.A., Reina, J.I., (2006) Mon. Not. R. Astron. Soc., 371 (4), p. 1873http://purl.org/coar/resource_type/c_c94fTHUMBNAILMiniProdInv.pngMiniProdInv.pngimage/png23941https://repositorio.utb.edu.co/bitstream/20.500.12585/9114/1/MiniProdInv.png0cb0f101a8d16897fb46fc914d3d7043MD5120.500.12585/9114oai:repositorio.utb.edu.co:20.500.12585/91142023-05-26 11:44:08.938Repositorio Institucional UTBrepositorioutb@utb.edu.co |
dc.title.none.fl_str_mv |
An infinite family of relativistic magnetized finite thin disks |
title |
An infinite family of relativistic magnetized finite thin disks |
spellingShingle |
An infinite family of relativistic magnetized finite thin disks Magnetic fields Maxwell equations Einstein Maxwell equations Energy condition Energy-momentum tensor Oblate spheroidal coordinates Physical quantities Thin disk Relativity |
title_short |
An infinite family of relativistic magnetized finite thin disks |
title_full |
An infinite family of relativistic magnetized finite thin disks |
title_fullStr |
An infinite family of relativistic magnetized finite thin disks |
title_full_unstemmed |
An infinite family of relativistic magnetized finite thin disks |
title_sort |
An infinite family of relativistic magnetized finite thin disks |
dc.subject.keywords.none.fl_str_mv |
Magnetic fields Maxwell equations Einstein Maxwell equations Energy condition Energy-momentum tensor Oblate spheroidal coordinates Physical quantities Thin disk Relativity |
topic |
Magnetic fields Maxwell equations Einstein Maxwell equations Energy condition Energy-momentum tensor Oblate spheroidal coordinates Physical quantities Thin disk Relativity |
description |
An infinite family of relativistic finite thin disk model with magnetic field is presented. The model is obtained for solving the Einstein-Maxwell equations for static spacetimes by means of the Horsk-Mitskievitch generating conjecture. The vacuum limit of these obtained solutions is the well known Morgan and Morgan solution. The obtained expressions are simply written in terms of oblate spheroidal coordinates. The mass of the disks are finite and the energy-momentum tensor agrees with all the energy conditions. The magnetic field and the circular velocity are evaluated explicitly. All the physical quantities obtained shown an acceptable behavior © Published under licence by IOP Publishing Ltd. |
publishDate |
2011 |
dc.date.issued.none.fl_str_mv |
2011 |
dc.date.accessioned.none.fl_str_mv |
2020-03-26T16:32:59Z |
dc.date.available.none.fl_str_mv |
2020-03-26T16:32:59Z |
dc.type.coarversion.fl_str_mv |
http://purl.org/coar/version/c_970fb48d4fbd8a85 |
dc.type.coar.fl_str_mv |
http://purl.org/coar/resource_type/c_c94f |
dc.type.driver.none.fl_str_mv |
info:eu-repo/semantics/conferenceObject |
dc.type.hasversion.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.spa.none.fl_str_mv |
Conferencia |
status_str |
publishedVersion |
dc.identifier.citation.none.fl_str_mv |
Journal of Physics: Conference Series; Vol. 314, Núm. 1 |
dc.identifier.issn.none.fl_str_mv |
17426588 |
dc.identifier.uri.none.fl_str_mv |
https://hdl.handle.net/20.500.12585/9114 |
dc.identifier.doi.none.fl_str_mv |
10.1088/1742-6596/314/1/012090 |
dc.identifier.instname.none.fl_str_mv |
Universidad Tecnológica de Bolívar |
dc.identifier.reponame.none.fl_str_mv |
Repositorio UTB |
dc.identifier.orcid.none.fl_str_mv |
54397050000 7202571265 |
identifier_str_mv |
Journal of Physics: Conference Series; Vol. 314, Núm. 1 17426588 10.1088/1742-6596/314/1/012090 Universidad Tecnológica de Bolívar Repositorio UTB 54397050000 7202571265 |
url |
https://hdl.handle.net/20.500.12585/9114 |
dc.language.iso.none.fl_str_mv |
eng |
language |
eng |
dc.relation.conferenceplace.none.fl_str_mv |
Granada |
dc.relation.conferencedate.none.fl_str_mv |
6 September 2010 through 10 September 2010 |
dc.rights.coar.fl_str_mv |
http://purl.org/coar/access_right/c_16ec |
dc.rights.uri.none.fl_str_mv |
http://creativecommons.org/licenses/by-nc-nd/4.0/ |
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info:eu-repo/semantics/restrictedAccess |
dc.rights.cc.none.fl_str_mv |
Atribución-NoComercial 4.0 Internacional |
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http://creativecommons.org/licenses/by-nc-nd/4.0/ Atribución-NoComercial 4.0 Internacional http://purl.org/coar/access_right/c_16ec |
eu_rights_str_mv |
restrictedAccess |
dc.format.medium.none.fl_str_mv |
Recurso electrónico |
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application/pdf |
dc.publisher.none.fl_str_mv |
Institute of Physics Publishing |
publisher.none.fl_str_mv |
Institute of Physics Publishing |
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https://www.scopus.com/inward/record.uri?eid=2-s2.0-81455154977&doi=10.1088%2f1742-6596%2f314%2f1%2f012090&partnerID=40&md5=1766de214272a8963422289e2233df12 |
institution |
Universidad Tecnológica de Bolívar |
dc.source.event.none.fl_str_mv |
Spanish Relativity Meeting: Gravity as a Crossroad in Physics, ERE 2010 |
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