Please use this identifier to cite or link to this item:
https://repositorio.accefyn.org.co/handle/001/1187
Cómo citar
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Granda, Luis N. | - |
dc.date.accessioned | 2021-12-10T08:12:52Z | - |
dc.date.available | 2021-12-10T08:12:52Z | - |
dc.date.issued | 2020-03-25 | - |
dc.identifier.uri | https://repositorio.accefyn.org.co/handle/001/1187 | - |
dc.description.abstract | Se estudian soluciones cosmológicas para un campo escalar acoplado mínimamente a la curvatura, en el marco del principio holográfico. Se pueden obtener soluciones phantom sin introducir grados de libertad fantasma, y el sistema autónomo contiene soluciones de expansión acelerada estables y atractores de Sitter. Para el campo con acoplamiento no-mínimo se analiza el caso especial del acoplamiento conforme y se demuestra que un campo escalar que evoluciona dinámicamente puede producir el efecto de la constante cosmológica. | spa |
dc.description.abstract | We study cosmological solutions for a scalar field minimally coupled to the curvature, in the framework of holographic dark energy. Phantom solutions can be obtained without introducing ghosts’ degrees of freedom, and the autonomous system contains stable accelerated expansion solutions and de Sitter attractors. For the non-minimally coupled scalar field the special case of the conformal coupling is analyzed, and it is shown that dynamically evolving scalar field produces the effect of the cosmological constant. | eng |
dc.format.mimetype | application/pdf | spa |
dc.language.iso | spa | spa |
dc.publisher | Academia Colombiana de Ciencias Exactas, Físicas y Naturales | spa |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International | spa |
dc.rights.uri | https://creativecommons.org/licenses/by-nc/4.0/ | spa |
dc.source | Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales | spa |
dc.title | The Scalar Field Model of Dark Energy in the Framework of the Holographic Principle | spa |
dc.type | Artículo de revista | spa |
dcterms.audience | Estudiantes, Profesores, Comunidad científica colombiana | spa |
dcterms.references | Ade, P. A. R., et al. (2016). Planck 2015 Results. XIII. Cosmological Parameters. Astron. And Astrophys., 594: 1-63. DOI: https://doi.org/10.1051/0004-6361/201525830 | spa |
dcterms.references | Arkani-Hamed, N., Cheng, H., Luty, M. A., Mukohyama, S. (2004). Ghost Condensation and consistent infrared Modification of Gravity. JHEP 0405, 074: 1-35. | spa |
dcterms.references | Armendariz-Picon, C., Mukhanov, V., Steinhardt, P. J. (2000). A dynamical solution to the problem of a small cosmological constant and late-time cosmic acceleration, Phys. Rev. Lett., 85: 4438-4421. | spa |
dcterms.references | Birrell, N.D. and Davis, P.C.W. (1982). Quantum fields in curved space-time. Cambridge, United Kingdom: Cambridge University Press | spa |
dcterms.references | Bousso, R. (1999). A Covariant Entropy Conjecture. JHEP. 9907: 1-33 | spa |
dcterms.references | Caldwell, R. R. (2002). A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of state. Phys. Lett. B. 545: 23-29. | spa |
dcterms.references | Cohen, A., Kaplan, D., Nelson, A. (1999). Effective Field Theory, Black Holes, and the Cosmological Constant. Phys. Rev. Lett. 82: 4971-4974 | spa |
dcterms.references | Ford, L.H. (1987). Gravitational Particle creation and Inflation. Phys. Rev. D35: 2955-2960 | spa |
dcterms.references | Granda, L. N., Jimenez, D. F. (2017). Dynamical Analysis for a Scalar-Tensor Model with Gauss- Bonnet and Non-Minimal couplings. Eur. Phys. J. C. 77, 679: 1-12. | spa |
dcterms.references | Granda, L. N., Jimenez, D. F. (2018). Dynamical Analysis for a Scalar-Tensor Model with Kinetic and Non-Minimal couplings. IJMPD 27, 1850030: 1-22. | spa |
dcterms.references | Granda, L. N., Oliveros, A. (2008). Infrared Cut-off Proposal for the Holographic Density. Phys. Lett. B 669: 275-277 | spa |
dcterms.references | Granda, L. N., Oliveros, A. (2008a). New Infrared Cut-off for the Holographic Scalar Fields Models of Dark Energy. Phys. Lett. B 671: 199-202 | spa |
dcterms.references | Hicken, M. et al. (2009). Improved dark Energy Constraints from ~100 New CFA Supernova Type Ia Light Curves. Astrophys. J. 700: 1097-1140 | spa |
dcterms.references | Hsu, S. D. (2004). Entropy Bounds and Dark Energy. Phys. Lett. B 594: 13-16 | spa |
dcterms.references | Ito, M. (2005). Holographic Dark Energy Model with Non-minimal Coupling. Europhys. Lett. 71: 712-715. | spa |
dcterms.references | Kowalski, M. et al. (2008). Improved Cosmological Constraints from New, Old and Combined Supernova Datasets. Astrophys. Journal, 686: 749-778 | spa |
dcterms.references | Padmanabhan, T., Choudhury, T. R. (2002). Can the Clustered dark matter and the smooth dark energy arise from the same scalar field? Phys. Rev. D 66: 081301 | spa |
dcterms.references | Perlmutter, S. et al. (1988). Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Constant. Nature. 391: 51-54. | spa |
dcterms.references | Perivolaropoulos, L. (2005). Crossing the Phantom Divide Barrier with Scalar-Tensor Theories. JCAP 0510, 001: 1-16 | spa |
dcterms.references | Ratra, B., Peebles, J. (1988). Cosmological consequences of a rolling homogeneous scalar field. Phys. Rev. D37: 3406-3427 | spa |
dcterms.references | Riess, A.G. et al. (1998). Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant. Astron. J. 116: 1009-1038 | spa |
dcterms.references | Sami, M., Shahalam, M., Skugoreva, M., Toporensky, A. (2012). Cosmological Dynamics of Non-Minimally Coupled scalar Field system and Its late Time Cosmic Relevance. Phys. Rev. D 86, 103532: 1-17. | spa |
dcterms.references | Setare, M.R., Saridakis, E.N. (2009). Non-minimally Coupled Canonical, Phantom and Quintom Models of Holographic Dark Energy. Phys. Lett. B671: 331-338 | spa |
dcterms.references | Susskind, L. (1995). The World as a Hologram. J. Math. Phys. 36: 6377-6396. | spa |
dcterms.references | ‘t Hooft, G. (1993). Dimensional Reduction in Quantum Gravity. arXiv:gr-qc/9310026 | spa |
dc.rights.accessrights | info:eu-repo/semantics/openAccess | spa |
dc.type.driver | info:eu-repo/semantics/article | spa |
dc.type.version | info:eu-repo/semantics/publishedVersion | spa |
dc.rights.creativecommons | Atribución-NoComercial 4.0 Internacional (CC BY-NC 4.0) | spa |
dc.identifier.doi | https://doi.org/10.18257/raccefyn.966 | - |
dc.subject.proposal | Energía Oscura | spa |
dc.subject.proposal | Dark Energy | eng |
dc.subject.proposal | Principio Holográfico | spa |
dc.subject.proposal | Holographic Principle | eng |
dc.subject.proposal | Campo escalar | spa |
dc.subject.proposal | Scalar Field | eng |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | spa |
dc.relation.ispartofjournal | Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales | spa |
dc.relation.citationvolume | 44 | spa |
dc.relation.citationstartpage | 133 | spa |
dc.relation.citationendpage | 141 | spa |
dc.publisher.place | Bogotá, Colombia | spa |
dc.contributor.corporatename | Academia Colombiana de Ciencias Exactas, Físicas y Naturales | spa |
dc.relation.citationissue | 170 | spa |
dc.type.content | DataPaper | spa |
dc.type.redcol | http://purl.org/redcol/resource_type/ART | spa |
oaire.accessrights | http://purl.org/coar/access_right/c_abf2 | spa |
oaire.version | http://purl.org/coar/version/c_970fb48d4fbd8a85 | spa |
Appears in Collections: | BA. Revista de la Academia Colombiana de Ciencias Exactas Físicas y Naturales |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
5. The Scalar Field Model of Dark Energy.pdf | Ciencias físicas | 950.11 kB | Adobe PDF | View/Open |
This item is licensed under a Creative Commons License