Time variation of fundamental constants in nonstandard cosmological models
- Autores
- Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- In this work we have studied the lithium problem in nonstandard cosmological models. In particular, by using the public code ALTERBBN, we have included in the computation of the primordial light nuclei abundances, the effects of the inclusion of dark energy and dark entropy, along with the variation of the fine structure constant and the Higgs vacuum expectation value. In order to set constrains on the variation of the fundamental constants we have compared our theoretical results with the available observational data. We have found that the lithium abundance is reduced for not-null variation at the 3σ-level of both constants.
Facultad de Ciencias Astronómicas y Geofísicas
Facultad de Ciencias Exactas - Materia
-
Física
Nonstandard cosmological models
Lithium - 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:10915/118368
Ver los metadatos del registro completo
id |
SEDICI_b2bd8b591f56b7f9777ef39ff00fea3e |
---|---|
oai_identifier_str |
oai:sedici.unlp.edu.ar:10915/118368 |
network_acronym_str |
SEDICI |
repository_id_str |
1329 |
network_name_str |
SEDICI (UNLP) |
spelling |
Time variation of fundamental constants in nonstandard cosmological modelsMosquera, Mercedes ElisaCivitarese, Enrique OsvaldoFísicaNonstandard cosmological modelsLithiumIn this work we have studied the lithium problem in nonstandard cosmological models. In particular, by using the public code ALTERBBN, we have included in the computation of the primordial light nuclei abundances, the effects of the inclusion of dark energy and dark entropy, along with the variation of the fine structure constant and the Higgs vacuum expectation value. In order to set constrains on the variation of the fundamental constants we have compared our theoretical results with the available observational data. We have found that the lithium abundance is reduced for not-null variation at the 3σ-level of both constants.Facultad de Ciencias Astronómicas y GeofísicasFacultad de Ciencias Exactas2017info: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/10915/118368enginfo:eu-repo/semantics/altIdentifier/issn/2469-9985info:eu-repo/semantics/altIdentifier/issn/2469-9993info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevC.96.045802info: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:UNLP2025-09-29T11:27:50Zoai:sedici.unlp.edu.ar:10915/118368Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:27:50.795SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Time variation of fundamental constants in nonstandard cosmological models |
title |
Time variation of fundamental constants in nonstandard cosmological models |
spellingShingle |
Time variation of fundamental constants in nonstandard cosmological models Mosquera, Mercedes Elisa Física Nonstandard cosmological models Lithium |
title_short |
Time variation of fundamental constants in nonstandard cosmological models |
title_full |
Time variation of fundamental constants in nonstandard cosmological models |
title_fullStr |
Time variation of fundamental constants in nonstandard cosmological models |
title_full_unstemmed |
Time variation of fundamental constants in nonstandard cosmological models |
title_sort |
Time variation of fundamental constants in nonstandard cosmological models |
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 |
Física Nonstandard cosmological models Lithium |
topic |
Física Nonstandard cosmological models Lithium |
dc.description.none.fl_txt_mv |
In this work we have studied the lithium problem in nonstandard cosmological models. In particular, by using the public code ALTERBBN, we have included in the computation of the primordial light nuclei abundances, the effects of the inclusion of dark energy and dark entropy, along with the variation of the fine structure constant and the Higgs vacuum expectation value. In order to set constrains on the variation of the fundamental constants we have compared our theoretical results with the available observational data. We have found that the lithium abundance is reduced for not-null variation at the 3σ-level of both constants. Facultad de Ciencias Astronómicas y Geofísicas Facultad de Ciencias Exactas |
description |
In this work we have studied the lithium problem in nonstandard cosmological models. In particular, by using the public code ALTERBBN, we have included in the computation of the primordial light nuclei abundances, the effects of the inclusion of dark energy and dark entropy, along with the variation of the fine structure constant and the Higgs vacuum expectation value. In order to set constrains on the variation of the fundamental constants we have compared our theoretical results with the available observational data. We have found that the lithium abundance is reduced for not-null variation at the 3σ-level of both constants. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017 |
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/10915/118368 |
url |
http://sedici.unlp.edu.ar/handle/10915/118368 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/2469-9985 info:eu-repo/semantics/altIdentifier/issn/2469-9993 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevC.96.045802 |
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 |
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 |
_version_ |
1844616156901539840 |
score |
13.070432 |