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
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/95564

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network_name_str SEDICI (UNLP)
spelling 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
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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