Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach
- Autores
- Landau, Susana Judith; Mosquera, Mercedes Elisa; Vucetich, Héctor
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Using the semi-analytic method proposed by Esmaizaldeh and coworkers we calculate the abundances of the light elements produced during primordial nucleosynthesis assuming that the gauge coupling constants of the fundamental interactions may vary. We analyze the dependence of the nucleon masses, nuclear binding energies and cross sections involved in the calculation of the abundances with the fundamental constants assuming the chiral limit of QCD. We obtain the abundances of light elements as a function of the fundamental constants. Finally, using the observational data of d, 3He, 4He and 7Li we estimate constraints on the variation of the fundamental constants between the time of primordial nucleosynthesis and the present. All observational abundances and the WMAP estimate of the baryon density can be fitted to the theoretical predictions with varying coupling constants. The possible systematic errors in the observational data preclude stronger conclusions.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Astronomía
Física
Ciencias Exactas
Cosmologicla parameters
Early universe
Nuclear reactions
Nucleosyntesis abundances - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/95564
Ver los metadatos del registro completo
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Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical ApproachLandau, Susana JudithMosquera, Mercedes ElisaVucetich, HéctorAstronomíaFísicaCiencias ExactasCosmologicla parametersEarly universeNuclear reactionsNucleosyntesis abundancesUsing the semi-analytic method proposed by Esmaizaldeh and coworkers we calculate the abundances of the light elements produced during primordial nucleosynthesis assuming that the gauge coupling constants of the fundamental interactions may vary. We analyze the dependence of the nucleon masses, nuclear binding energies and cross sections involved in the calculation of the abundances with the fundamental constants assuming the chiral limit of QCD. We obtain the abundances of light elements as a function of the fundamental constants. Finally, using the observational data of d, <sup>3</sup>He, <sup>4</sup>He and <sup>7</sup>Li we estimate constraints on the variation of the fundamental constants between the time of primordial nucleosynthesis and the present. All observational abundances and the WMAP estimate of the baryon density can be fitted to the theoretical predictions with varying coupling constants. The possible systematic errors in the observational data preclude stronger conclusions.Facultad de Ciencias Astronómicas y Geofísicas2006-01-20info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf38-52http://sedici.unlp.edu.ar/handle/10915/95564enginfo:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/73310info:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/431417info:eu-repo/semantics/altIdentifier/hdl/11336/73310info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/2.5/ar/Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:12:15Zoai:sedici.unlp.edu.ar:10915/95564Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:12:15.347SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
title |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
spellingShingle |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach Landau, Susana Judith Astronomía Física Ciencias Exactas Cosmologicla parameters Early universe Nuclear reactions Nucleosyntesis abundances |
title_short |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
title_full |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
title_fullStr |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
title_full_unstemmed |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
title_sort |
Primordial Nucleosynthesis with Varying Fundamental Constants : A Semianalytical Approach |
dc.creator.none.fl_str_mv |
Landau, Susana Judith Mosquera, Mercedes Elisa Vucetich, Héctor |
author |
Landau, Susana Judith |
author_facet |
Landau, Susana Judith Mosquera, Mercedes Elisa Vucetich, Héctor |
author_role |
author |
author2 |
Mosquera, Mercedes Elisa Vucetich, Héctor |
author2_role |
author author |
dc.subject.none.fl_str_mv |
Astronomía Física Ciencias Exactas Cosmologicla parameters Early universe Nuclear reactions Nucleosyntesis abundances |
topic |
Astronomía Física Ciencias Exactas Cosmologicla parameters Early universe Nuclear reactions Nucleosyntesis abundances |
dc.description.none.fl_txt_mv |
Using the semi-analytic method proposed by Esmaizaldeh and coworkers we calculate the abundances of the light elements produced during primordial nucleosynthesis assuming that the gauge coupling constants of the fundamental interactions may vary. We analyze the dependence of the nucleon masses, nuclear binding energies and cross sections involved in the calculation of the abundances with the fundamental constants assuming the chiral limit of QCD. We obtain the abundances of light elements as a function of the fundamental constants. Finally, using the observational data of d, <sup>3</sup>He, <sup>4</sup>He and <sup>7</sup>Li we estimate constraints on the variation of the fundamental constants between the time of primordial nucleosynthesis and the present. All observational abundances and the WMAP estimate of the baryon density can be fitted to the theoretical predictions with varying coupling constants. The possible systematic errors in the observational data preclude stronger conclusions. Facultad de Ciencias Astronómicas y Geofísicas |
description |
Using the semi-analytic method proposed by Esmaizaldeh and coworkers we calculate the abundances of the light elements produced during primordial nucleosynthesis assuming that the gauge coupling constants of the fundamental interactions may vary. We analyze the dependence of the nucleon masses, nuclear binding energies and cross sections involved in the calculation of the abundances with the fundamental constants assuming the chiral limit of QCD. We obtain the abundances of light elements as a function of the fundamental constants. Finally, using the observational data of d, <sup>3</sup>He, <sup>4</sup>He and <sup>7</sup>Li we estimate constraints on the variation of the fundamental constants between the time of primordial nucleosynthesis and the present. All observational abundances and the WMAP estimate of the baryon density can be fitted to the theoretical predictions with varying coupling constants. The possible systematic errors in the observational data preclude stronger conclusions. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-01-20 |
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/10915/95564 |
url |
http://sedici.unlp.edu.ar/handle/10915/95564 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://ri.conicet.gov.ar/11336/73310 info:eu-repo/semantics/altIdentifier/issn/0004-637X info:eu-repo/semantics/altIdentifier/doi/10.1086/431417 info:eu-repo/semantics/altIdentifier/hdl/11336/73310 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by-nc-sa/2.5/ar/ Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by-nc-sa/2.5/ar/ Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Argentina (CC BY-NC-SA 2.5) |
dc.format.none.fl_str_mv |
application/pdf 38-52 |
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reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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