Calculation of primordial abundances of light nuclei including a heavy sterile neutrino
- Autores
- Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We include the coupling of a heavy sterile neutrino with active neutrinos in the calculation of primordial abundances of light-nuclei. We calculate neutrino distribution functions and primordial abundances, as functions depending on a renormalization of the sterile neutrino distribution function (a), the sterile neutrino mass (ms) and the mixing angle (φ). Using the observable data, we set constrains on these parameters, which have the values a < 0.4, sin2 φ ≈ 0.12-0.39 and ms < 7 keV at 1σ level, for a fixed value of the baryon to photon ratio. When the baryon to photon ratio is allowed to vary, its extracted value is in agreement with the values constrained by Planck observations and by the Wilkinson Microwave Anisotropy Probe (WMAP). It is found that the anomaly in the abundance of 7Li persists, in spite of the inclusion of a heavy sterile neutrino.
Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Civitarese, Enrique Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina - Materia
-
BIG BANG NUCLEOSYNTHESIS
NEUTRINO MASSES FROM COSMOLOGY
NEUTRINO PROPERTIES - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/53475
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Calculation of primordial abundances of light nuclei including a heavy sterile neutrinoMosquera, Mercedes ElisaCivitarese, Enrique OsvaldoBIG BANG NUCLEOSYNTHESISNEUTRINO MASSES FROM COSMOLOGYNEUTRINO PROPERTIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We include the coupling of a heavy sterile neutrino with active neutrinos in the calculation of primordial abundances of light-nuclei. We calculate neutrino distribution functions and primordial abundances, as functions depending on a renormalization of the sterile neutrino distribution function (a), the sterile neutrino mass (ms) and the mixing angle (φ). Using the observable data, we set constrains on these parameters, which have the values a < 0.4, sin2 φ ≈ 0.12-0.39 and ms < 7 keV at 1σ level, for a fixed value of the baryon to photon ratio. When the baryon to photon ratio is allowed to vary, its extracted value is in agreement with the values constrained by Planck observations and by the Wilkinson Microwave Anisotropy Probe (WMAP). It is found that the anomaly in the abundance of 7Li persists, in spite of the inclusion of a heavy sterile neutrino.Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Civitarese, Enrique Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaIOP Publishing2015-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/53475Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Calculation of primordial abundances of light nuclei including a heavy sterile neutrino; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2015; 8; 8-2015; 1-141475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2015/08/038info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1475-7516/2015/08/038/metainfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1411.4030info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:00:34Zoai:ri.conicet.gov.ar:11336/53475instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:00:34.952CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
title |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
spellingShingle |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino Mosquera, Mercedes Elisa BIG BANG NUCLEOSYNTHESIS NEUTRINO MASSES FROM COSMOLOGY NEUTRINO PROPERTIES |
title_short |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
title_full |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
title_fullStr |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
title_full_unstemmed |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
title_sort |
Calculation of primordial abundances of light nuclei including a heavy sterile neutrino |
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 |
BIG BANG NUCLEOSYNTHESIS NEUTRINO MASSES FROM COSMOLOGY NEUTRINO PROPERTIES |
topic |
BIG BANG NUCLEOSYNTHESIS NEUTRINO MASSES FROM COSMOLOGY NEUTRINO PROPERTIES |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We include the coupling of a heavy sterile neutrino with active neutrinos in the calculation of primordial abundances of light-nuclei. We calculate neutrino distribution functions and primordial abundances, as functions depending on a renormalization of the sterile neutrino distribution function (a), the sterile neutrino mass (ms) and the mixing angle (φ). Using the observable data, we set constrains on these parameters, which have the values a < 0.4, sin2 φ ≈ 0.12-0.39 and ms < 7 keV at 1σ level, for a fixed value of the baryon to photon ratio. When the baryon to photon ratio is allowed to vary, its extracted value is in agreement with the values constrained by Planck observations and by the Wilkinson Microwave Anisotropy Probe (WMAP). It is found that the anomaly in the abundance of 7Li persists, in spite of the inclusion of a heavy sterile neutrino. Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Civitarese, Enrique Osvaldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina |
description |
We include the coupling of a heavy sterile neutrino with active neutrinos in the calculation of primordial abundances of light-nuclei. We calculate neutrino distribution functions and primordial abundances, as functions depending on a renormalization of the sterile neutrino distribution function (a), the sterile neutrino mass (ms) and the mixing angle (φ). Using the observable data, we set constrains on these parameters, which have the values a < 0.4, sin2 φ ≈ 0.12-0.39 and ms < 7 keV at 1σ level, for a fixed value of the baryon to photon ratio. When the baryon to photon ratio is allowed to vary, its extracted value is in agreement with the values constrained by Planck observations and by the Wilkinson Microwave Anisotropy Probe (WMAP). It is found that the anomaly in the abundance of 7Li persists, in spite of the inclusion of a heavy sterile neutrino. |
publishDate |
2015 |
dc.date.none.fl_str_mv |
2015-08 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 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://hdl.handle.net/11336/53475 Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Calculation of primordial abundances of light nuclei including a heavy sterile neutrino; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2015; 8; 8-2015; 1-14 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/53475 |
identifier_str_mv |
Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Calculation of primordial abundances of light nuclei including a heavy sterile neutrino; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2015; 8; 8-2015; 1-14 1475-7516 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2015/08/038 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/1475-7516/2015/08/038/meta info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1411.4030 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.070432 |