On classical thermal stability of black holes with a dynamical extrinsic curvature
We study the deformation caused by the influence of the extrinsic curvature on a vacuum spherically symmetric metric embedded in a five-dimensional bulk. We investigate the resulting black-holes obtaining general characteristics such as their masses, horizons, singularities and thermal properties by...
- Autores:
- Tipo de recurso:
- Fecha de publicación:
- 2017
- Institución:
- Universidad Tecnológica de Bolívar
- Repositorio:
- Repositorio Institucional UTB
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.utb.edu.co:20.500.12585/8934
- Acceso en línea:
- https://hdl.handle.net/20.500.12585/8934
- Palabra clave:
- Black holes
Classical BH's thermodynamics
Dynamical embedding
Extra-dimensions
Extrinsic geometry
- Rights
- restrictedAccess
- License
- http://creativecommons.org/licenses/by-nc-nd/4.0/
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On classical thermal stability of black holes with a dynamical extrinsic curvature |
| title |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| spellingShingle |
On classical thermal stability of black holes with a dynamical extrinsic curvature Black holes Classical BH's thermodynamics Dynamical embedding Extra-dimensions Extrinsic geometry |
| title_short |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| title_full |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| title_fullStr |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| title_full_unstemmed |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| title_sort |
On classical thermal stability of black holes with a dynamical extrinsic curvature |
| dc.subject.keywords.none.fl_str_mv |
Black holes Classical BH's thermodynamics Dynamical embedding Extra-dimensions Extrinsic geometry |
| topic |
Black holes Classical BH's thermodynamics Dynamical embedding Extra-dimensions Extrinsic geometry |
| description |
We study the deformation caused by the influence of the extrinsic curvature on a vacuum spherically symmetric metric embedded in a five-dimensional bulk. We investigate the resulting black-holes obtaining general characteristics such as their masses, horizons, singularities and thermal properties by using a dynamical extrinsic curvature leading to different results as those from rigid embedded models. As a test, we also study the bending of light near such black-holes analyzing the movement of a test particle and the modification caused by extrinsic curvature on its movement. Accordingly, using the asymptotically conformal flat condition, we show that such black holes must be large and constrained by the allowed number range −1/2≤n≤1.8 for a set of n-scalar potentials. As a result, they are locally thermodynamically stable, but not globally preferred. © 2017 Elsevier Inc. |
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2017 |
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2017 |
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2020-03-26T16:32:37Z |
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2020-03-26T16:32:37Z |
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http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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info:eu-repo/semantics/article |
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Artículo |
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publishedVersion |
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Annals of Physics; Vol. 380, pp. 106-120 |
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00034916 |
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https://hdl.handle.net/20.500.12585/8934 |
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10.1016/j.aop.2017.03.006 |
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Universidad Tecnológica de Bolívar |
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Repositorio UTB |
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26530767700 25225467000 15763870900 15753419400 |
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Annals of Physics; Vol. 380, pp. 106-120 00034916 10.1016/j.aop.2017.03.006 Universidad Tecnológica de Bolívar Repositorio UTB 26530767700 25225467000 15763870900 15753419400 |
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https://hdl.handle.net/20.500.12585/8934 |
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eng |
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eng |
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info:eu-repo/semantics/restrictedAccess |
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Atribución-NoComercial 4.0 Internacional |
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Recurso electrónico |
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application/pdf |
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Academic Press Inc. |
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Academic Press Inc. |
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2020-03-26T16:32:37Z2020-03-26T16:32:37Z2017Annals of Physics; Vol. 380, pp. 106-12000034916https://hdl.handle.net/20.500.12585/893410.1016/j.aop.2017.03.006Universidad Tecnológica de BolívarRepositorio UTB26530767700252254670001576387090015753419400We study the deformation caused by the influence of the extrinsic curvature on a vacuum spherically symmetric metric embedded in a five-dimensional bulk. We investigate the resulting black-holes obtaining general characteristics such as their masses, horizons, singularities and thermal properties by using a dynamical extrinsic curvature leading to different results as those from rigid embedded models. As a test, we also study the bending of light near such black-holes analyzing the movement of a test particle and the modification caused by extrinsic curvature on its movement. Accordingly, using the asymptotically conformal flat condition, we show that such black holes must be large and constrained by the allowed number range −1/2≤n≤1.8 for a set of n-scalar potentials. As a result, they are locally thermodynamically stable, but not globally preferred. © 2017 Elsevier Inc.Recurso electrónicoapplication/pdfengAcademic Press Inc.http://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-s2.0-85016553092&doi=10.1016%2fj.aop.2017.03.006&partnerID=40&md5=74269a9263c0ea721625ada0a680dbd3On classical thermal stability of black holes with a dynamical extrinsic curvatureinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1Black holesClassical BH's thermodynamicsDynamical embeddingExtra-dimensionsExtrinsic geometryCapistrano A.J.S.Gutiérrez-Piñeres A.C.Ulhoa S.C.Amorim R.G.G.Capistrano, A.J.S., Cabral, L.A., (2014) Ann. Phys., 384, pp. 64-83Maia, M.D., Monte, E.M., Maia, J.M.F., Alcaniz, J.S., (2005) Classical Quantum Gravity, 22, p. 1623Maia, M.D., Capistrano, A.J.S., Alcaniz, J.S., Monte, E.M., (2011) Gen. Relativity Gravitation, 10, p. 2685Maia, M.D., Silva, N., Fernandes, M.C.B., (2007) J. High Energy Phys., 4, p. 047Nash, J., (1956) Ann. of Math., 63, p. 20Randall, L., Sundrum, R., (1999) Phys. Rev. Lett., 83, p. 3370Randall, L., Sundrum, R., (1999) Phys. Rev. Lett., 83, p. 4690Israel, W., (1966) Il Nuovo Cimento, 44 (2), pp. 1-14Arkani-Hamed, N., (1998) Phys. Lett. B, 429, p. 263Dvali, G., Gabadadze, G., Porrati, M., (2000) Phys. Lett. B, 485 (1-3), pp. 208-214Battye, R.A., Carter, B., (2001) Phys. Lett. B, 509, p. 331Maia, M.D., Monte, E.M., (2002) Phys. Lett. A, 297 (2), pp. 9-19Heydari-Fard, M., Sepangi, H.R., (2007) Phys. Lett. B, 649, pp. 1-11Jalalzadeh, S., Mehrnia, M., Sepangi, H.R., (2009) Classical Quantum Gravity, 26Ranjbar, A., Sepangi, H.R., Shahidi, S., (2012) Ann. 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B, 647, pp. 472-476http://purl.org/coar/resource_type/c_6501THUMBNAILMiniProdInv.pngMiniProdInv.pngimage/png23941https://repositorio.utb.edu.co/bitstream/20.500.12585/8934/1/MiniProdInv.png0cb0f101a8d16897fb46fc914d3d7043MD5120.500.12585/8934oai:repositorio.utb.edu.co:20.500.12585/89342021-02-02 15:09:45.531Repositorio Institucional UTBrepositorioutb@utb.edu.co |