Neutrinos in large extra dimensions and short-baseline νe appearance

Detalhes bibliográficos
Autor(a) principal: Carena, Marcela
Data de Publicação: 2017
Outros Autores: Li, Ying-Ying, MacHado, Camila S., MacHado, Pedro A. N., Wagner, Carlos E. M.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.96.095014
http://hdl.handle.net/11449/220978
Resumo: We show that, in the presence of bulk masses, sterile neutrinos propagating in large extra dimensions (LED) can induce electron-neutrino appearance effects. This is in contrast to what happens in the standard LED scenario, and hence LED models with explicit bulk masses have the potential to address the MiniBooNE and LSND appearance results as well as the reactor and Gallium anomalies. A special feature in our scenario is that the mixing of the first Kaluza-Klein modes to active neutrinos can be suppressed, making the contribution of heavier sterile neutrinos to oscillations relatively more important. We study the implications of this neutrino mass generation mechanism for current and future neutrino oscillation experiments and show that the Short Baseline Neutrino Program at Fermilab will be able to efficiently probe such a scenario. In addition, this framework leads to massive Dirac neutrinos and thus precludes any signal in neutrinoless double beta decay experiments.
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spelling Neutrinos in large extra dimensions and short-baseline νe appearanceWe show that, in the presence of bulk masses, sterile neutrinos propagating in large extra dimensions (LED) can induce electron-neutrino appearance effects. This is in contrast to what happens in the standard LED scenario, and hence LED models with explicit bulk masses have the potential to address the MiniBooNE and LSND appearance results as well as the reactor and Gallium anomalies. A special feature in our scenario is that the mixing of the first Kaluza-Klein modes to active neutrinos can be suppressed, making the contribution of heavier sterile neutrinos to oscillations relatively more important. We study the implications of this neutrino mass generation mechanism for current and future neutrino oscillation experiments and show that the Short Baseline Neutrino Program at Fermilab will be able to efficiently probe such a scenario. In addition, this framework leads to massive Dirac neutrinos and thus precludes any signal in neutrinoless double beta decay experiments.Theoretical Physics Department Fermi National Accelerator Laboratory, P.O. Box 500Enrico Fermi Institute University of ChicagoKavli Institute for Cosmological Physics University of ChicagoDepartment of Physics Hong Kong University of Science and Technology, Clear Water BayInstituto de Física Teórica Universidade EstadualHigh Energy Physics Division Argonne National LaboratoryFermi National Accelerator LaboratoryUniversity of ChicagoHong Kong University of Science and TechnologyUniversidade EstadualArgonne National LaboratoryCarena, MarcelaLi, Ying-YingMacHado, Camila S.MacHado, Pedro A. N.Wagner, Carlos E. M.2022-04-28T19:07:10Z2022-04-28T19:07:10Z2017-11-16info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.96.095014Physical Review D, v. 96, n. 9, 2017.2470-00292470-0010http://hdl.handle.net/11449/22097810.1103/PhysRevD.96.0950142-s2.0-85037709744Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-28T19:07:10Zoai:repositorio.unesp.br:11449/220978Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-28T19:07:10Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Neutrinos in large extra dimensions and short-baseline νe appearance
title Neutrinos in large extra dimensions and short-baseline νe appearance
spellingShingle Neutrinos in large extra dimensions and short-baseline νe appearance
Carena, Marcela
title_short Neutrinos in large extra dimensions and short-baseline νe appearance
title_full Neutrinos in large extra dimensions and short-baseline νe appearance
title_fullStr Neutrinos in large extra dimensions and short-baseline νe appearance
title_full_unstemmed Neutrinos in large extra dimensions and short-baseline νe appearance
title_sort Neutrinos in large extra dimensions and short-baseline νe appearance
author Carena, Marcela
author_facet Carena, Marcela
Li, Ying-Ying
MacHado, Camila S.
MacHado, Pedro A. N.
Wagner, Carlos E. M.
author_role author
author2 Li, Ying-Ying
MacHado, Camila S.
MacHado, Pedro A. N.
Wagner, Carlos E. M.
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Fermi National Accelerator Laboratory
University of Chicago
Hong Kong University of Science and Technology
Universidade Estadual
Argonne National Laboratory
dc.contributor.author.fl_str_mv Carena, Marcela
Li, Ying-Ying
MacHado, Camila S.
MacHado, Pedro A. N.
Wagner, Carlos E. M.
description We show that, in the presence of bulk masses, sterile neutrinos propagating in large extra dimensions (LED) can induce electron-neutrino appearance effects. This is in contrast to what happens in the standard LED scenario, and hence LED models with explicit bulk masses have the potential to address the MiniBooNE and LSND appearance results as well as the reactor and Gallium anomalies. A special feature in our scenario is that the mixing of the first Kaluza-Klein modes to active neutrinos can be suppressed, making the contribution of heavier sterile neutrinos to oscillations relatively more important. We study the implications of this neutrino mass generation mechanism for current and future neutrino oscillation experiments and show that the Short Baseline Neutrino Program at Fermilab will be able to efficiently probe such a scenario. In addition, this framework leads to massive Dirac neutrinos and thus precludes any signal in neutrinoless double beta decay experiments.
publishDate 2017
dc.date.none.fl_str_mv 2017-11-16
2022-04-28T19:07:10Z
2022-04-28T19:07:10Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.96.095014
Physical Review D, v. 96, n. 9, 2017.
2470-0029
2470-0010
http://hdl.handle.net/11449/220978
10.1103/PhysRevD.96.095014
2-s2.0-85037709744
url http://dx.doi.org/10.1103/PhysRevD.96.095014
http://hdl.handle.net/11449/220978
identifier_str_mv Physical Review D, v. 96, n. 9, 2017.
2470-0029
2470-0010
10.1103/PhysRevD.96.095014
2-s2.0-85037709744
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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