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No-go limitations on UV completions of the Neutrino Option

We discuss the possible origin of the Majorana mass scale(s) required for the “neutrino option” where the electroweak scale is generated simultaneously with light neutrino masses in a type-I seesaw model by common dimension four interactions. We establish no-go constraints on the perturbative genera...

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Detalles Bibliográficos
Autores principales: Brivio, Ilaria, Talbert, Jim, Trott, Michael
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.103.015012
http://cds.cern.ch/record/2744912
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author Brivio, Ilaria
Talbert, Jim
Trott, Michael
author_facet Brivio, Ilaria
Talbert, Jim
Trott, Michael
author_sort Brivio, Ilaria
collection CERN
description We discuss the possible origin of the Majorana mass scale(s) required for the “neutrino option” where the electroweak scale is generated simultaneously with light neutrino masses in a type-I seesaw model by common dimension four interactions. We establish no-go constraints on the perturbative generation of the Majorana masses required due to global symmetries of the seesaw Lagrangian.
id cern-2744912
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
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spelling cern-27449122023-10-12T06:01:12Zdoi:10.1103/PhysRevD.103.015012http://cds.cern.ch/record/2744912engBrivio, IlariaTalbert, JimTrott, MichaelNo-go limitations on UV completions of the Neutrino Optionhep-phParticle Physics - PhenomenologyWe discuss the possible origin of the Majorana mass scale(s) required for the “neutrino option” where the electroweak scale is generated simultaneously with light neutrino masses in a type-I seesaw model by common dimension four interactions. We establish no-go constraints on the perturbative generation of the Majorana masses required due to global symmetries of the seesaw Lagrangian.We discuss the possible origin of the Majorana mass scale(s) required for the "Neutrino Option" where the electroweak scale is generated simultaneously with light neutrino masses in a type-I seesaw model, by common dimension four interactions. We establish no-go constraints on the perturbative generation of the Majorana masses required due to global symmetries of the seesaw Lagrangian.arXiv:2010.15428oai:cds.cern.ch:27449122020-10-29
spellingShingle hep-ph
Particle Physics - Phenomenology
Brivio, Ilaria
Talbert, Jim
Trott, Michael
No-go limitations on UV completions of the Neutrino Option
title No-go limitations on UV completions of the Neutrino Option
title_full No-go limitations on UV completions of the Neutrino Option
title_fullStr No-go limitations on UV completions of the Neutrino Option
title_full_unstemmed No-go limitations on UV completions of the Neutrino Option
title_short No-go limitations on UV completions of the Neutrino Option
title_sort no-go limitations on uv completions of the neutrino option
topic hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.103.015012
http://cds.cern.ch/record/2744912
work_keys_str_mv AT brivioilaria nogolimitationsonuvcompletionsoftheneutrinooption
AT talbertjim nogolimitationsonuvcompletionsoftheneutrinooption
AT trottmichael nogolimitationsonuvcompletionsoftheneutrinooption