Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile...

Full description

Bibliographic Details
Authors: Aiello, S, Albert, A., Alves Garre, Sergio, Ameli, F, André, Michel|||0000-0002-0091-7279, Androulakis, Giorgos, Anghinolfi, Marco, Anguita, M., Ardid Ramírez, Miguel, Aublin, J., Bagatelas, Christos, Baret, B., van den Berg, A.M., Bertin, Vincent, Biagi, S., Bouwhuis, M.C., Brunner, J., Busto, José
Format: article
Publication Date:2021
Country:España
Institution:Universitat Politècnica de Catalunya (UPC)
Repository:UPCommons. Portal del coneixement obert de la UPC
Language:English
OAI Identifier:oai:upcommons.upc.edu:2117/360554
Online Access:https://hdl.handle.net/2117/360554
https://dx.doi.org/10.1007/JHEP10(2021)180
Access Level:Open access
Keyword:Telescopes
Neutrinos
Neutrino astrophysics
Astronomy -- Observations
Neutrino
Detectors and Telescopes (experiments)
Oscillation
Neutrins
Astrofísica
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
id ES_0685f32bbc70843dcff220a2e897bf59
oai_identifier_str oai:upcommons.upc.edu:2117/360554
network_acronym_str ES
network_name_str España
repository_id_str
spelling Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCAAiello, SAlbert, A.Alves Garre, SergioAmeli, FAndré, Michel|||0000-0002-0091-7279Androulakis, GiorgosAnghinolfi, MarcoAnguita, M.Ardid Ramírez, MiguelAublin, J.Bagatelas, ChristosBaret, B.van den Berg, A.M.Bertin, VincentBiagi, S.Bouwhuis, M.C.Brunner, J.Busto, JoséTelescopesNeutrinosNeutrino astrophysicsAstronomy -- ObservationsNeutrinoDetectors and Telescopes (experiments)OscillationNeutrinsAstrofísicaÀrees temàtiques de la UPC::Física::Astronomia i astrofísicaKM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles θ14, θ24, θ34 and the effective angle θµe, over a broad range of mass squared difference ∆m2 41 „ r10´5 , 10s eV2 , allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurementsPeer ReviewedSpringer20212021-10-2120222022-01-25journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/2117/360554https://dx.doi.org/10.1007/JHEP10(2021)180reponame:UPCommons. Portal del coneixement obert de la UPCinstname:Universitat Politècnica de Catalunya (UPC)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Attribution-NonCommercial-NoDerivs 3.0 Spainhttp://creativecommons.org/licenses/by-nc-nd/3.0/es/info:eu-repo/semantics/openAccessoai:upcommons.upc.edu:2117/3605542026-05-27T15:37:01Z
dc.title.none.fl_str_mv Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
title Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
spellingShingle Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
Aiello, S
Telescopes
Neutrinos
Neutrino astrophysics
Astronomy -- Observations
Neutrino
Detectors and Telescopes (experiments)
Oscillation
Neutrins
Astrofísica
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
title_short Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
title_full Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
title_fullStr Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
title_full_unstemmed Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
title_sort Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
dc.creator.none.fl_str_mv Aiello, S
Albert, A.
Alves Garre, Sergio
Ameli, F
André, Michel|||0000-0002-0091-7279
Androulakis, Giorgos
Anghinolfi, Marco
Anguita, M.
Ardid Ramírez, Miguel
Aublin, J.
Bagatelas, Christos
Baret, B.
van den Berg, A.M.
Bertin, Vincent
Biagi, S.
Bouwhuis, M.C.
Brunner, J.
Busto, José
author Aiello, S
author_facet Aiello, S
Albert, A.
Alves Garre, Sergio
Ameli, F
André, Michel|||0000-0002-0091-7279
Androulakis, Giorgos
Anghinolfi, Marco
Anguita, M.
Ardid Ramírez, Miguel
Aublin, J.
Bagatelas, Christos
Baret, B.
van den Berg, A.M.
Bertin, Vincent
Biagi, S.
Bouwhuis, M.C.
Brunner, J.
Busto, José
author_role author
author2 Albert, A.
Alves Garre, Sergio
Ameli, F
André, Michel|||0000-0002-0091-7279
Androulakis, Giorgos
Anghinolfi, Marco
Anguita, M.
Ardid Ramírez, Miguel
Aublin, J.
Bagatelas, Christos
Baret, B.
van den Berg, A.M.
Bertin, Vincent
Biagi, S.
Bouwhuis, M.C.
Brunner, J.
Busto, José
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Telescopes
Neutrinos
Neutrino astrophysics
Astronomy -- Observations
Neutrino
Detectors and Telescopes (experiments)
Oscillation
Neutrins
Astrofísica
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
topic Telescopes
Neutrinos
Neutrino astrophysics
Astronomy -- Observations
Neutrino
Detectors and Telescopes (experiments)
Oscillation
Neutrins
Astrofísica
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
description KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles θ14, θ24, θ34 and the effective angle θµe, over a broad range of mass squared difference ∆m2 41 „ r10´5 , 10s eV2 , allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements
publishDate 2021
dc.date.none.fl_str_mv 2021
2021-10-21
2022
2022-01-25
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/2117/360554
https://dx.doi.org/10.1007/JHEP10(2021)180
url https://hdl.handle.net/2117/360554
https://dx.doi.org/10.1007/JHEP10(2021)180
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution-NonCommercial-NoDerivs 3.0 Spain
http://creativecommons.org/licenses/by-nc-nd/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv reponame:UPCommons. Portal del coneixement obert de la UPC
instname:Universitat Politècnica de Catalunya (UPC)
instname_str Universitat Politècnica de Catalunya (UPC)
reponame_str UPCommons. Portal del coneixement obert de la UPC
collection UPCommons. Portal del coneixement obert de la UPC
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869402923077730304
score 15,300719

Similar Items