On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses
- Autores
- Roulet, Esteban; Vissani, Francesco
- Año de publicación
- 2018
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The capture rates of non-relativistic neutrinos on beta decaying nuclei depends on whether their mass is Dirac or Majorana. It is known that for relic neutrinos from the big-bang, and within minimal assumptions, the rate is a factor two larger in the Majorana case. We show that this difference also depends on the value of the lightest neutrino mass and on the type of mass hierarchy. If the lightest neutrino has a mass below the meV, so that it is still relativistic today, its capture rate for the case of Dirac masses becomes equal to that for Majorana masses. As a consequence, for the case of normal neutrino mass hierarchy, for which the total capture rate is dominated by the contribution from the lightest neutrino, if this one is below the meV the distinction between the Dirac and Majorana scenarios can only rely on the detection of the two heavier neutrinos, which is something very challenging.
Fil: Roulet, Esteban. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina
Fil: Vissani, Francesco. Laboratori Nazionali del Gran Sasso; Italia - Materia
-
COSMOLOGICAL NEUTRINOS
NEUTRINO EXPER- IMENTS
PARTICLE PHYSICS - COSMOLOGY CONNECTION - 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:11336/112549
Ver los metadatos del registro completo
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On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypothesesRoulet, EstebanVissani, FrancescoCOSMOLOGICAL NEUTRINOSNEUTRINO EXPER- IMENTSPARTICLE PHYSICS - COSMOLOGY CONNECTIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The capture rates of non-relativistic neutrinos on beta decaying nuclei depends on whether their mass is Dirac or Majorana. It is known that for relic neutrinos from the big-bang, and within minimal assumptions, the rate is a factor two larger in the Majorana case. We show that this difference also depends on the value of the lightest neutrino mass and on the type of mass hierarchy. If the lightest neutrino has a mass below the meV, so that it is still relativistic today, its capture rate for the case of Dirac masses becomes equal to that for Majorana masses. As a consequence, for the case of normal neutrino mass hierarchy, for which the total capture rate is dominated by the contribution from the lightest neutrino, if this one is below the meV the distinction between the Dirac and Majorana scenarios can only rely on the detection of the two heavier neutrinos, which is something very challenging.Fil: Roulet, Esteban. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; ArgentinaFil: Vissani, Francesco. Laboratori Nazionali del Gran Sasso; ItaliaIOP Publishing2018-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/112549Roulet, Esteban; Vissani, Francesco; On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2018; 10; 10-2018; 1-121475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1475-7516/2018/10/049info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2018/10/049info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:43:09Zoai:ri.conicet.gov.ar:11336/112549instacron: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 09:43:09.743CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
title |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
spellingShingle |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses Roulet, Esteban COSMOLOGICAL NEUTRINOS NEUTRINO EXPER- IMENTS PARTICLE PHYSICS - COSMOLOGY CONNECTION |
title_short |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
title_full |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
title_fullStr |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
title_full_unstemmed |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
title_sort |
On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses |
dc.creator.none.fl_str_mv |
Roulet, Esteban Vissani, Francesco |
author |
Roulet, Esteban |
author_facet |
Roulet, Esteban Vissani, Francesco |
author_role |
author |
author2 |
Vissani, Francesco |
author2_role |
author |
dc.subject.none.fl_str_mv |
COSMOLOGICAL NEUTRINOS NEUTRINO EXPER- IMENTS PARTICLE PHYSICS - COSMOLOGY CONNECTION |
topic |
COSMOLOGICAL NEUTRINOS NEUTRINO EXPER- IMENTS PARTICLE PHYSICS - COSMOLOGY CONNECTION |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The capture rates of non-relativistic neutrinos on beta decaying nuclei depends on whether their mass is Dirac or Majorana. It is known that for relic neutrinos from the big-bang, and within minimal assumptions, the rate is a factor two larger in the Majorana case. We show that this difference also depends on the value of the lightest neutrino mass and on the type of mass hierarchy. If the lightest neutrino has a mass below the meV, so that it is still relativistic today, its capture rate for the case of Dirac masses becomes equal to that for Majorana masses. As a consequence, for the case of normal neutrino mass hierarchy, for which the total capture rate is dominated by the contribution from the lightest neutrino, if this one is below the meV the distinction between the Dirac and Majorana scenarios can only rely on the detection of the two heavier neutrinos, which is something very challenging. Fil: Roulet, Esteban. Comisión Nacional de Energía Atómica. Centro Atómico Bariloche; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Patagonia Norte; Argentina Fil: Vissani, Francesco. Laboratori Nazionali del Gran Sasso; Italia |
description |
The capture rates of non-relativistic neutrinos on beta decaying nuclei depends on whether their mass is Dirac or Majorana. It is known that for relic neutrinos from the big-bang, and within minimal assumptions, the rate is a factor two larger in the Majorana case. We show that this difference also depends on the value of the lightest neutrino mass and on the type of mass hierarchy. If the lightest neutrino has a mass below the meV, so that it is still relativistic today, its capture rate for the case of Dirac masses becomes equal to that for Majorana masses. As a consequence, for the case of normal neutrino mass hierarchy, for which the total capture rate is dominated by the contribution from the lightest neutrino, if this one is below the meV the distinction between the Dirac and Majorana scenarios can only rely on the detection of the two heavier neutrinos, which is something very challenging. |
publishDate |
2018 |
dc.date.none.fl_str_mv |
2018-10 |
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/11336/112549 Roulet, Esteban; Vissani, Francesco; On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2018; 10; 10-2018; 1-12 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/112549 |
identifier_str_mv |
Roulet, Esteban; Vissani, Francesco; On the capture rates of big bang neutrinos by nuclei within the Dirac and Majorana hypotheses; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2018; 10; 10-2018; 1-12 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/url/https://iopscience.iop.org/article/10.1088/1475-7516/2018/10/049 info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2018/10/049 |
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 |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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