Nuclear and particle physics aspects of Big Bang nucleo-synthesis
- Autores
- Civitarese, Enrique Osvaldo; Mosquera, Mercedes Elisa
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Big Bang Nucleo Synthesis (BBN) is the process which has occurred during the first three minutes of the Universe, that is during the time it needed to cooled down to temperatures of the order of 109 K. The standard BBN model depends on one parameter, the baryonic density, and it is one of the proper tools to study the physics of the Universe at its earliest stage. In this paper we shall discuss the rol of BBN as a testing ground for evidences and possible limits which could be determined from cosmological analysis based on the inclusion of sterile neutrinos, the variation of the mass of the Higgs boson and the time variation of fundamental constant.
Facultad de Ciencias Exactas
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Física
Astronomía
Big Bang Nucleo Synthesis (BBN) - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83928
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Nuclear and particle physics aspects of Big Bang nucleo-synthesisCivitarese, Enrique OsvaldoMosquera, Mercedes ElisaFísicaAstronomíaBig Bang Nucleo Synthesis (BBN)Big Bang Nucleo Synthesis (BBN) is the process which has occurred during the first three minutes of the Universe, that is during the time it needed to cooled down to temperatures of the order of 109 K. The standard BBN model depends on one parameter, the baryonic density, and it is one of the proper tools to study the physics of the Universe at its earliest stage. In this paper we shall discuss the rol of BBN as a testing ground for evidences and possible limits which could be determined from cosmological analysis based on the inclusion of sterile neutrinos, the variation of the mass of the Higgs boson and the time variation of fundamental constant.Facultad de Ciencias ExactasFacultad de Ciencias Astronómicas y Geofísicas2011info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/83928enginfo:eu-repo/semantics/altIdentifier/issn/1742-6588info:eu-repo/semantics/altIdentifier/doi/10.1088/1742-6596/322/1/012005info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:08:02Zoai:sedici.unlp.edu.ar:10915/83928Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:08:02.963SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
title |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
spellingShingle |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis Civitarese, Enrique Osvaldo Física Astronomía Big Bang Nucleo Synthesis (BBN) |
title_short |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
title_full |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
title_fullStr |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
title_full_unstemmed |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
title_sort |
Nuclear and particle physics aspects of Big Bang nucleo-synthesis |
dc.creator.none.fl_str_mv |
Civitarese, Enrique Osvaldo Mosquera, Mercedes Elisa |
author |
Civitarese, Enrique Osvaldo |
author_facet |
Civitarese, Enrique Osvaldo Mosquera, Mercedes Elisa |
author_role |
author |
author2 |
Mosquera, Mercedes Elisa |
author2_role |
author |
dc.subject.none.fl_str_mv |
Física Astronomía Big Bang Nucleo Synthesis (BBN) |
topic |
Física Astronomía Big Bang Nucleo Synthesis (BBN) |
dc.description.none.fl_txt_mv |
Big Bang Nucleo Synthesis (BBN) is the process which has occurred during the first three minutes of the Universe, that is during the time it needed to cooled down to temperatures of the order of 109 K. The standard BBN model depends on one parameter, the baryonic density, and it is one of the proper tools to study the physics of the Universe at its earliest stage. In this paper we shall discuss the rol of BBN as a testing ground for evidences and possible limits which could be determined from cosmological analysis based on the inclusion of sterile neutrinos, the variation of the mass of the Higgs boson and the time variation of fundamental constant. Facultad de Ciencias Exactas Facultad de Ciencias Astronómicas y Geofísicas |
description |
Big Bang Nucleo Synthesis (BBN) is the process which has occurred during the first three minutes of the Universe, that is during the time it needed to cooled down to temperatures of the order of 109 K. The standard BBN model depends on one parameter, the baryonic density, and it is one of the proper tools to study the physics of the Universe at its earliest stage. In this paper we shall discuss the rol of BBN as a testing ground for evidences and possible limits which could be determined from cosmological analysis based on the inclusion of sterile neutrinos, the variation of the mass of the Higgs boson and the time variation of fundamental constant. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011 |
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http://sedici.unlp.edu.ar/handle/10915/83928 |
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eng |
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eng |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
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