Time variation of the electron mass in the early universe and the Barrow-Magueijo model

Autores
Scóccola, Claudia Graciela; Mosquera, Mercedes Elisa; Landau, Susana Judith; Vucetich, Héctor
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We put limits on the time variation of the electron mass in the early universe using observational primordial abundances of D, 4He, and 7Li, recent data from the cosmic microwave background, and the 2dFGRS power spectrum. Furthermore, we use these constraints together with other astronomical and geophysical bounds from the late universe to test the Barrow-Magueijo model for the variation in me. From our analysis we obtain -0.615 < Gω/c4 < -0.045 (3 σ interval), in disagreement with the result obtained in the original paper.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
Materia
Ciencias Astronómicas
Cosmic microwave background
Cosmology: Theory
Early universe
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/84151
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/84151
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Time variation of the electron mass in the early universe and the Barrow-Magueijo modelScóccola, Claudia GracielaMosquera, Mercedes ElisaLandau, Susana JudithVucetich, HéctorCiencias AstronómicasCosmic microwave backgroundCosmology: TheoryEarly universeWe put limits on the time variation of the electron mass in the early universe using observational primordial abundances of D, <SUP>4</SUP>He, and <SUP>7</SUP>Li, recent data from the cosmic microwave background, and the 2dFGRS power spectrum. Furthermore, we use these constraints together with other astronomical and geophysical bounds from the late universe to test the Barrow-Magueijo model for the variation in m<SUB>e</SUB>. From our analysis we obtain -0.615 < Gω/c<SUP>4</SUP> < -0.045 (3 σ interval), in disagreement with the result obtained in the original paper.Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2008info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf737-746http://sedici.unlp.edu.ar/handle/10915/84151enginfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/588086info: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:UNLP2025-09-29T11:16:11Zoai:sedici.unlp.edu.ar:10915/84151Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:16:11.454SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Time variation of the electron mass in the early universe and the Barrow-Magueijo model
title Time variation of the electron mass in the early universe and the Barrow-Magueijo model
spellingShingle Time variation of the electron mass in the early universe and the Barrow-Magueijo model
Scóccola, Claudia Graciela
Ciencias Astronómicas
Cosmic microwave background
Cosmology: Theory
Early universe
title_short Time variation of the electron mass in the early universe and the Barrow-Magueijo model
title_full Time variation of the electron mass in the early universe and the Barrow-Magueijo model
title_fullStr Time variation of the electron mass in the early universe and the Barrow-Magueijo model
title_full_unstemmed Time variation of the electron mass in the early universe and the Barrow-Magueijo model
title_sort Time variation of the electron mass in the early universe and the Barrow-Magueijo model
dc.creator.none.fl_str_mv Scóccola, Claudia Graciela
Mosquera, Mercedes Elisa
Landau, Susana Judith
Vucetich, Héctor
author Scóccola, Claudia Graciela
author_facet Scóccola, Claudia Graciela
Mosquera, Mercedes Elisa
Landau, Susana Judith
Vucetich, Héctor
author_role author
author2 Mosquera, Mercedes Elisa
Landau, Susana Judith
Vucetich, Héctor
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Cosmic microwave background
Cosmology: Theory
Early universe
topic Ciencias Astronómicas
Cosmic microwave background
Cosmology: Theory
Early universe
dc.description.none.fl_txt_mv We put limits on the time variation of the electron mass in the early universe using observational primordial abundances of D, <SUP>4</SUP>He, and <SUP>7</SUP>Li, recent data from the cosmic microwave background, and the 2dFGRS power spectrum. Furthermore, we use these constraints together with other astronomical and geophysical bounds from the late universe to test the Barrow-Magueijo model for the variation in m<SUB>e</SUB>. From our analysis we obtain -0.615 < Gω/c<SUP>4</SUP> < -0.045 (3 σ interval), in disagreement with the result obtained in the original paper.
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata
description We put limits on the time variation of the electron mass in the early universe using observational primordial abundances of D, <SUP>4</SUP>He, and <SUP>7</SUP>Li, recent data from the cosmic microwave background, and the 2dFGRS power spectrum. Furthermore, we use these constraints together with other astronomical and geophysical bounds from the late universe to test the Barrow-Magueijo model for the variation in m<SUB>e</SUB>. From our analysis we obtain -0.615 < Gω/c<SUP>4</SUP> < -0.045 (3 σ interval), in disagreement with the result obtained in the original paper.
publishDate 2008
dc.date.none.fl_str_mv 2008
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/10915/84151
url http://sedici.unlp.edu.ar/handle/10915/84151
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0004-637X
info:eu-repo/semantics/altIdentifier/doi/10.1086/588086
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
737-746
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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score 13.070432

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