A no-hair theorem for black holes in f(R) gravity
In this work we present a no-hair theorem which discards the existence of four-dimensional asymptotically flat, static and spherically symmetric or stationary axisymmetric, non-trivial black holes in the frame of f (R) gravity under metric formalism. Here we show that our no-hair theorem also can di...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2018
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/8892
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/8892
- Palabra clave:
- Black-hole solutions
Modified theories of gravity
No-hair theorems
- Rights
- restrictedAccess
- License
- http://creativecommons.org/licenses/by-nc-nd/4.0/
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A no-hair theorem for black holes in f(R) gravity |
| title |
A no-hair theorem for black holes in f(R) gravity |
| spellingShingle |
A no-hair theorem for black holes in f(R) gravity Black-hole solutions Modified theories of gravity No-hair theorems |
| title_short |
A no-hair theorem for black holes in f(R) gravity |
| title_full |
A no-hair theorem for black holes in f(R) gravity |
| title_fullStr |
A no-hair theorem for black holes in f(R) gravity |
| title_full_unstemmed |
A no-hair theorem for black holes in f(R) gravity |
| title_sort |
A no-hair theorem for black holes in f(R) gravity |
| dc.subject.keywords.none.fl_str_mv |
Black-hole solutions Modified theories of gravity No-hair theorems |
| topic |
Black-hole solutions Modified theories of gravity No-hair theorems |
| description |
In this work we present a no-hair theorem which discards the existence of four-dimensional asymptotically flat, static and spherically symmetric or stationary axisymmetric, non-trivial black holes in the frame of f (R) gravity under metric formalism. Here we show that our no-hair theorem also can discard asymptotic de Sitter stationary and axisymmetric non-trivial black holes. The novelty is that this no-hair theorem is built without resorting to known mapping between f (R) gravity and scalar-tensor theory. Thus, an advantage will be that our no-hair theorem applies as well to metric f (R) models that cannot be mapped to scalar-tensor theory. © 2017 IOP Publishing Ltd. |
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2018 |
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2018 |
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2020-03-26T16:32:34Z |
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2020-03-26T16:32:34Z |
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Artículo |
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Classical and Quantum Gravity; Vol. 35, Núm. 2 |
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02649381 |
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https://hdl.handle.net/20.500.12585/8892 |
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10.1088/1361-6382/aa8e2e |
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Universidad Tecnológica de Bolívar |
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Repositorio UTB |
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55744418600 |
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Classical and Quantum Gravity; Vol. 35, Núm. 2 02649381 10.1088/1361-6382/aa8e2e Universidad Tecnológica de Bolívar Repositorio UTB 55744418600 |
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https://hdl.handle.net/20.500.12585/8892 |
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eng |
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2020-03-26T16:32:34Z2020-03-26T16:32:34Z2018Classical and Quantum Gravity; Vol. 35, Núm. 202649381https://hdl.handle.net/20.500.12585/889210.1088/1361-6382/aa8e2eUniversidad Tecnológica de BolívarRepositorio UTB55744418600In this work we present a no-hair theorem which discards the existence of four-dimensional asymptotically flat, static and spherically symmetric or stationary axisymmetric, non-trivial black holes in the frame of f (R) gravity under metric formalism. Here we show that our no-hair theorem also can discard asymptotic de Sitter stationary and axisymmetric non-trivial black holes. The novelty is that this no-hair theorem is built without resorting to known mapping between f (R) gravity and scalar-tensor theory. Thus, an advantage will be that our no-hair theorem applies as well to metric f (R) models that cannot be mapped to scalar-tensor theory. © 2017 IOP Publishing Ltd.Consejo Nacional de Ciencia y TecnologíaThe author acknowledges Nora Breton for useful discussions and suggestions to improve this manuscript, and also Luisa G Jaime and Marcelo Salgado for many valuable discussions. This work was supported in part by the CONACyT.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-s2.0-85039731115&doi=10.1088%2f1361-6382%2faa8e2e&partnerID=40&md5=3b34c15edfe59c6f27753bceca314abbA no-hair theorem for black holes in f(R) gravityinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1Black-hole solutionsModified theories of gravityNo-hair theoremsCañate P.Wald, R.M., (1984) General Relativity, , (Chicago, IL: Chicago University Press)Utiyama, R., DeWitt, B.S., (1962) J. Math. Phys., 3, p. 608Stelle, K.S., (1977) Phys. Rev., 16, p. 953Felice, A.D., Tsujikawa, S., (2010) Living Rev. 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