New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value
- Autores
- Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Aims. We study the time variation of the fine structure constant, α, and the Higgs vacuum expectation value v, during the Big Bang nucleosynthesis (BBN). Methods. We computed primordial abundances of light nuclei produced during the BBN stage by including resonances in the leading reaction rates which reduce the primordial abundance of beryllium. We performed this calculation considering that α and v may vary during the BBN. Using observable data on deuterium, 4He, and 7Li, we set constraints on the variation of the fundamental constants. Results. Results indicate a null variation of α and v, while the best-fit value for the baryon-to-photon ratio agrees well with the WMAP value. Conclusions. We found that the variation of α is null within 3σ, the variation of v is null within 6σ, and the preferred value of the baryon-to-photon ratio is in good agreement, within 3σ, with the value extracted using the WMAP data. We improve the fits respect to previous works.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Cosmological parameters
Cosmology: miscellaneous
Primordial nucleosynthesis - 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:10915/85229
Ver los metadatos del registro completo
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New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation valueMosquera, Mercedes ElisaCivitarese, Enrique OsvaldoCiencias AstronómicasCosmological parametersCosmology: miscellaneousPrimordial nucleosynthesisAims. We study the time variation of the fine structure constant, α, and the Higgs vacuum expectation value v, during the Big Bang nucleosynthesis (BBN). Methods. We computed primordial abundances of light nuclei produced during the BBN stage by including resonances in the leading reaction rates which reduce the primordial abundance of beryllium. We performed this calculation considering that α and v may vary during the BBN. Using observable data on deuterium, <SUP>4</SUP>He, and <SUP>7</SUP>Li, we set constraints on the variation of the fundamental constants. Results. Results indicate a null variation of α and v, while the best-fit value for the baryon-to-photon ratio agrees well with the WMAP value. Conclusions. We found that the variation of α is null within 3σ, the variation of v is null within 6σ, and the preferred value of the baryon-to-photon ratio is in good agreement, within 3σ, with the value extracted using the WMAP data. We improve the fits respect to previous works.Facultad de Ciencias Astronómicas y Geofísicas2013info: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/10915/85229enginfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220615info: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:UNLP2025-10-15T11:08:27Zoai:sedici.unlp.edu.ar:10915/85229Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:08:27.347SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
title |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
spellingShingle |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value Mosquera, Mercedes Elisa Ciencias Astronómicas Cosmological parameters Cosmology: miscellaneous Primordial nucleosynthesis |
title_short |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
title_full |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
title_fullStr |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
title_full_unstemmed |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
title_sort |
New cosmological constraints on the variation of fundamental constants: the fine structure constant and the Higgs vacuum expectation value |
dc.creator.none.fl_str_mv |
Mosquera, Mercedes Elisa Civitarese, Enrique Osvaldo |
author |
Mosquera, Mercedes Elisa |
author_facet |
Mosquera, Mercedes Elisa Civitarese, Enrique Osvaldo |
author_role |
author |
author2 |
Civitarese, Enrique Osvaldo |
author2_role |
author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Cosmological parameters Cosmology: miscellaneous Primordial nucleosynthesis |
topic |
Ciencias Astronómicas Cosmological parameters Cosmology: miscellaneous Primordial nucleosynthesis |
dc.description.none.fl_txt_mv |
Aims. We study the time variation of the fine structure constant, α, and the Higgs vacuum expectation value v, during the Big Bang nucleosynthesis (BBN). Methods. We computed primordial abundances of light nuclei produced during the BBN stage by including resonances in the leading reaction rates which reduce the primordial abundance of beryllium. We performed this calculation considering that α and v may vary during the BBN. Using observable data on deuterium, <SUP>4</SUP>He, and <SUP>7</SUP>Li, we set constraints on the variation of the fundamental constants. Results. Results indicate a null variation of α and v, while the best-fit value for the baryon-to-photon ratio agrees well with the WMAP value. Conclusions. We found that the variation of α is null within 3σ, the variation of v is null within 6σ, and the preferred value of the baryon-to-photon ratio is in good agreement, within 3σ, with the value extracted using the WMAP data. We improve the fits respect to previous works. Facultad de Ciencias Astronómicas y Geofísicas |
description |
Aims. We study the time variation of the fine structure constant, α, and the Higgs vacuum expectation value v, during the Big Bang nucleosynthesis (BBN). Methods. We computed primordial abundances of light nuclei produced during the BBN stage by including resonances in the leading reaction rates which reduce the primordial abundance of beryllium. We performed this calculation considering that α and v may vary during the BBN. Using observable data on deuterium, <SUP>4</SUP>He, and <SUP>7</SUP>Li, we set constraints on the variation of the fundamental constants. Results. Results indicate a null variation of α and v, while the best-fit value for the baryon-to-photon ratio agrees well with the WMAP value. Conclusions. We found that the variation of α is null within 3σ, the variation of v is null within 6σ, and the preferred value of the baryon-to-photon ratio is in good agreement, within 3σ, with the value extracted using the WMAP data. We improve the fits respect to previous works. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://sedici.unlp.edu.ar/handle/10915/85229 |
url |
http://sedici.unlp.edu.ar/handle/10915/85229 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6361 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220615 |
dc.rights.none.fl_str_mv |
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) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) |
dc.format.none.fl_str_mv |
application/pdf |
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reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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