Exact relativistic models of thin disks around static black holes in a magnetic field
The exact superposition of a central static black hole with surrounding thin disk in presence of a magnetic field is investigated. We consider two models of disk, one of infinite extension based on a Kuzmin-Chazy-Curzon metric and other finite based on the first Morgan-Morgan disk. We also analyze a...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2014
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/9067
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/9067
- Palabra clave:
- Einstein Maxwell equations
exact solution
General relativity
Thin disks
- Rights
- restrictedAccess
- License
- http://creativecommons.org/licenses/by-nc-nd/4.0/
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dc.title.none.fl_str_mv |
Exact relativistic models of thin disks around static black holes in a magnetic field |
title |
Exact relativistic models of thin disks around static black holes in a magnetic field |
spellingShingle |
Exact relativistic models of thin disks around static black holes in a magnetic field Einstein Maxwell equations exact solution General relativity Thin disks |
title_short |
Exact relativistic models of thin disks around static black holes in a magnetic field |
title_full |
Exact relativistic models of thin disks around static black holes in a magnetic field |
title_fullStr |
Exact relativistic models of thin disks around static black holes in a magnetic field |
title_full_unstemmed |
Exact relativistic models of thin disks around static black holes in a magnetic field |
title_sort |
Exact relativistic models of thin disks around static black holes in a magnetic field |
dc.subject.keywords.none.fl_str_mv |
Einstein Maxwell equations exact solution General relativity Thin disks |
topic |
Einstein Maxwell equations exact solution General relativity Thin disks |
description |
The exact superposition of a central static black hole with surrounding thin disk in presence of a magnetic field is investigated. We consider two models of disk, one of infinite extension based on a Kuzmin-Chazy-Curzon metric and other finite based on the first Morgan-Morgan disk. We also analyze a simple model of active galactic nuclei (AGN) consisting of black hole, a Kuzmin-Chazy-Curzon disk and two rods representing jets, in presence of magnetic field. To explain the stability of the disks, we consider the matter of the disk made of two pressureless streams of counter-rotating charged particles (counter-rotating model) moving along electrogeodesic. Using the Rayleigh criterion, we derivate for circular orbits the stability conditions of the particles of the streams. The influence of the magnetic field on the matter properties of the disk and on its stability are also analyzed. © World Scientific Publishing Company. |
publishDate |
2014 |
dc.date.issued.none.fl_str_mv |
2014 |
dc.date.accessioned.none.fl_str_mv |
2020-03-26T16:32:52Z |
dc.date.available.none.fl_str_mv |
2020-03-26T16:32:52Z |
dc.type.coarversion.fl_str_mv |
http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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info:eu-repo/semantics/article |
dc.type.hasVersion.none.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.spa.none.fl_str_mv |
Artículo |
status_str |
publishedVersion |
dc.identifier.citation.none.fl_str_mv |
International Journal of Modern Physics D; Vol. 23, Núm. 1 |
dc.identifier.issn.none.fl_str_mv |
02182718 |
dc.identifier.uri.none.fl_str_mv |
https://hdl.handle.net/20.500.12585/9067 |
dc.identifier.doi.none.fl_str_mv |
10.1142/S0218271814500102 |
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 |
25225467000 6506373811 7202571265 |
identifier_str_mv |
International Journal of Modern Physics D; Vol. 23, Núm. 1 02182718 10.1142/S0218271814500102 Universidad Tecnológica de Bolívar Repositorio UTB 25225467000 6506373811 7202571265 |
url |
https://hdl.handle.net/20.500.12585/9067 |
dc.language.iso.none.fl_str_mv |
eng |
language |
eng |
dc.rights.coar.fl_str_mv |
http://purl.org/coar/access_right/c_16ec |
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http://creativecommons.org/licenses/by-nc-nd/4.0/ |
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info:eu-repo/semantics/restrictedAccess |
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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 |
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restrictedAccess |
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Recurso electrónico |
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application/pdf |
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2020-03-26T16:32:52Z2020-03-26T16:32:52Z2014International Journal of Modern Physics D; Vol. 23, Núm. 102182718https://hdl.handle.net/20.500.12585/906710.1142/S0218271814500102Universidad Tecnológica de BolívarRepositorio UTB2522546700065063738117202571265The exact superposition of a central static black hole with surrounding thin disk in presence of a magnetic field is investigated. We consider two models of disk, one of infinite extension based on a Kuzmin-Chazy-Curzon metric and other finite based on the first Morgan-Morgan disk. We also analyze a simple model of active galactic nuclei (AGN) consisting of black hole, a Kuzmin-Chazy-Curzon disk and two rods representing jets, in presence of magnetic field. To explain the stability of the disks, we consider the matter of the disk made of two pressureless streams of counter-rotating charged particles (counter-rotating model) moving along electrogeodesic. Using the Rayleigh criterion, we derivate for circular orbits the stability conditions of the particles of the streams. The influence of the magnetic field on the matter properties of the disk and on its stability are also analyzed. © World Scientific Publishing Company.Recurso electrónicoapplication/pdfenghttp://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-s2.0-84891886579&doi=10.1142%2fS0218271814500102&partnerID=40&md5=2fcd66b5491b05f312977525547c9eadExact relativistic models of thin disks around static black holes in a magnetic fieldinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1Einstein Maxwell equationsexact solutionGeneral relativityThin disksGutiérrez-Piñeres A.C.García-Reyes G.González G.A.Kundt, W., (1996) Jets from Stars and Galactic Nuclei, Lecture Notes in Physics, 471. , (ed.) 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A, 93, p. 148Landau, L.D., Lifshitz, E.M., (1989) Fluid Mechanics, , Addison-Wesley, Reading, MALetelier, P.S., (2003) Phys. Rev. D, 68, p. 104002Kuzmin, G.G., (1956) Astron. Zh., 33, p. 27Toomre, A., (1962) Astrophys. J., 138, p. 385Chazy, J., (1924) Bull. Soc. Math. France, 52, p. 17Curzon, H.E.J., (1924) Proc. London Math. Soc., 23, p. 477Braithwaite, J., Spruit, H.C., (2004) Nature, 431, p. 819http://purl.org/coar/resource_type/c_6501THUMBNAILMiniProdInv.pngMiniProdInv.pngimage/png23941https://repositorio.utb.edu.co/bitstream/20.500.12585/9067/1/MiniProdInv.png0cb0f101a8d16897fb46fc914d3d7043MD5120.500.12585/9067oai:repositorio.utb.edu.co:20.500.12585/90672021-02-02 14:53:50.792Repositorio Institucional UTBrepositorioutb@utb.edu.co |