The KM3NeT potential for the next core-collapse supernova observation with neutrinos
[EN] The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with 6200 optical modules com...
Published in: | The European Physical Journal C |
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Main Authors: | , , , , , , , , , , , , , , , , , , , |
Other Authors: | , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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Springer-Verlag
2021
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Online Access: | http://hdl.handle.net/10251/184367 https://doi.org/10.1140/epjc/s10052-021-09187-5 |
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ftunivpvalencia:oai:riunet.upv.es:10251/184367 |
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openpolar |
institution |
Open Polar |
collection |
Politechnical University of Valencia: RiuNet |
op_collection_id |
ftunivpvalencia |
language |
English |
topic |
KM3NeT Core-collapse supernova Neutrinos FISICA APLICADA |
spellingShingle |
KM3NeT Core-collapse supernova Neutrinos FISICA APLICADA Aiello, S. Albert, A. Garre, S. Alves Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid Ramírez, Miguel Ardid-Ramírez, Joan Salvador Aublin, J. Bagatelas, C. Bou Cabo, Manuel Diego-Tortosa, Dídac Espinosa Roselló, Víctor Martínez Mora, Juan Antonio Poirè, Chiara The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
topic_facet |
KM3NeT Core-collapse supernova Neutrinos FISICA APLICADA |
description |
[EN] The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with 6200 optical modules comprising a total of 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to 10 MeV neutrinos from Galactic and near-Galactic core-collapse supernovae through the observation of coincident hits in photomultipliers above the background. In this paper, the sensitivity of KM3NeT to a supernova explosion is esti- mated from detailed analyses of background data from the first KM3NeT detection units and simulations of the neutrino signal. The KM3NeT observational horizon (for a 5 ¿ discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud (60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to deter- mine the arrival time of the neutrino burst with a few millisec- onds precision for sources up to 5¿8 kpc away, and detecting the peculiar signature of the standing accretion shock insta- bility if the core-collapse supernova explosion happens closer than 3¿5 kpc, depending on the progenitor mass. KM3NeT¿s capability to measure the neutrino flux spectral parameters is also presented. X The authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), ... |
author2 |
Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada European Commission Junta de Andalucía GENERALITAT VALENCIANA AGENCIA ESTATAL DE INVESTIGACION National Science Centre, Polonia Agencia Estatal de Investigación Agence Nationale de la Recherche, Francia Shota Rustaveli National Science Foundation Abdus Salam International Centre for Theoretical Physics Ministero dell'Istruzione dell'Università e della Ricerca Fundació Bancària Caixa d'Estalvis i Pensions de Barcelona |
format |
Article in Journal/Newspaper |
author |
Aiello, S. Albert, A. Garre, S. Alves Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid Ramírez, Miguel Ardid-Ramírez, Joan Salvador Aublin, J. Bagatelas, C. Bou Cabo, Manuel Diego-Tortosa, Dídac Espinosa Roselló, Víctor Martínez Mora, Juan Antonio Poirè, Chiara |
author_facet |
Aiello, S. Albert, A. Garre, S. Alves Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid Ramírez, Miguel Ardid-Ramírez, Joan Salvador Aublin, J. Bagatelas, C. Bou Cabo, Manuel Diego-Tortosa, Dídac Espinosa Roselló, Víctor Martínez Mora, Juan Antonio Poirè, Chiara |
author_sort |
Aiello, S. |
title |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_short |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_full |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_fullStr |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_full_unstemmed |
The KM3NeT potential for the next core-collapse supernova observation with neutrinos |
title_sort |
km3net potential for the next core-collapse supernova observation with neutrinos |
publisher |
Springer-Verlag |
publishDate |
2021 |
url |
http://hdl.handle.net/10251/184367 https://doi.org/10.1140/epjc/s10052-021-09187-5 |
long_lat |
ENVELOPE(-68.705,-68.705,-71.251,-71.251) |
geographic |
Milky Way |
geographic_facet |
Milky Way |
genre |
Orca |
genre_facet |
Orca |
op_relation |
The European Physical Journal C info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-A-C42/ES/CARACTERIZACION DEL FONDO ACUSTICO EN EL OBSERVATORIO SUBMARINO KM3NET/ info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/ info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C41/ES/FISICA FUNDAMENTAL Y ASTRONOMIA MULTIMENSAJERO CON TELESCOPIOS DE NEUTRINOS/ info:eu-repo/grantAgreement/Junta de Andalucía//SOMM17%2F6104%2FUGR / info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C43/ES/FISICA FUNDAMENTAL, DETECCION ACUSTICA Y ASTRONOMIA MULTI-MENSAJERO CON TELESCOPIOS DE NEUTRINOS EN LA UPV/ info:eu-repo/grantAgreement/ANR//ANR-18-IDEX-0001 / info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C44/ES/FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO CON TELESCOPIOS DE NEUTRINOS EN LA UGR/ info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2018%2F034 / info:eu-repo/grantAgreement/EC/H2020/713673/EU info:eu-repo/grantAgreement/ANR//ANR-15-CE31-0020/ info:eu-repo/grantAgreement/EC/H2020/739560/EU info:eu-repo/grantAgreement/ICTP//AF-13/ info:eu-repo/grantAgreement/NCN//2015%2F18%2FE%2FST2%2F00758 / info:eu-repo/grantAgreement/Fundació Bancària Caixa d'Estalvis i Pensions de Barcelona//LCF%2FBQ%2FIN17%2F11620019/ info:eu-repo/grantAgreement/MIUR//NAT-NET 2017W4HA7S/ info:eu-repo/grantAgreement/SRNSF//FR-18-1268/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//GRISOLIAP%2F2018%2F119//AYUDA SANTIAGO GRISOLIA PROYECTO: ACUSTICA EN DETECTORES DE PARTICULAS/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//CIDEGENT%2F2019%2F043//AYUDA CONTRATACION CIDEGENT INVESTIGADORES DE EXCELENCIA-ARDID RAMIREZ, JOAN/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//CIDEGENT%2F2019%2F043//ARTIFICIAL GENERAL INTELLIGENCE:BEYOND DEEP LEARNING/ https://doi.org/10.1140/epjc/s10052-021-09187-5 10.1093/acprof:oso/9780198508717.001.0001 10.1007/978-3-319-21846-5_109 10.1103/PhysRevD.38.448 10.1016/0168-9002(88)91097-2 10.1016/0370-2693(88)91651-6 10.1088/0954-3899/43/8/084001 10.1086/509773 10.1017/S1743921307000671 10.3847/1538-4357/aadcf7 10.1103/PhysRevD.90.045032 10.1103/PhysRevLett.111.121104 10.1103/PhysRevD.82.063007 10.1103/PhysRevD.99.063018 10.1103/PhysRevD.101.123013 10.1117/1.JATIS.5.4.046001 10.1140/epjc/s10052-014-3056-3 10.1140/epjc/s10052-015-3868-9 10.1051/0004-6361/201117810e 10.1146/annurev-nucl-102711-095006 10.1016/S0370-2693(03)00616-6 10.1142/S0217732393002567 10.1103/PhysRevD.66.013007 10.1016/j.nima.2010.06.258 10.1016/S0168-9002(03)01368-8 10.1140/epjc/s10052-020-7629-z 10.1016/j.astropartphys.2005.10.005 10.1086/305364 10.1393/ncr/i2016-10120-8 10.1140/epjc/s10052-011-1554-0 10.1140/epjc/s10052-013-2501-z |
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http://creativecommons.org/licenses/by/4.0/ info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.1140/epjc/s10052-021-09187-5 |
container_title |
The European Physical Journal C |
container_volume |
81 |
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5 |
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ftunivpvalencia:oai:riunet.upv.es:10251/184367 2024-01-28T10:08:28+01:00 The KM3NeT potential for the next core-collapse supernova observation with neutrinos Aiello, S. Albert, A. Garre, S. Alves Aly, Z. Ambrosone, A. Ameli, F. Andre, M. Androulakis, G. Anghinolfi, M. Anguita, M. Anton, G. Ardid Ramírez, Miguel Ardid-Ramírez, Joan Salvador Aublin, J. Bagatelas, C. Bou Cabo, Manuel Diego-Tortosa, Dídac Espinosa Roselló, Víctor Martínez Mora, Juan Antonio Poirè, Chiara Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada European Commission Junta de Andalucía GENERALITAT VALENCIANA AGENCIA ESTATAL DE INVESTIGACION National Science Centre, Polonia Agencia Estatal de Investigación Agence Nationale de la Recherche, Francia Shota Rustaveli National Science Foundation Abdus Salam International Centre for Theoretical Physics Ministero dell'Istruzione dell'Università e della Ricerca Fundació Bancària Caixa d'Estalvis i Pensions de Barcelona 2021-05 http://hdl.handle.net/10251/184367 https://doi.org/10.1140/epjc/s10052-021-09187-5 eng eng Springer-Verlag The European Physical Journal C info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-A-C42/ES/CARACTERIZACION DEL FONDO ACUSTICO EN EL OBSERVATORIO SUBMARINO KM3NET/ info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/ info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C41/ES/FISICA FUNDAMENTAL Y ASTRONOMIA MULTIMENSAJERO CON TELESCOPIOS DE NEUTRINOS/ info:eu-repo/grantAgreement/Junta de Andalucía//SOMM17%2F6104%2FUGR / info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C43/ES/FISICA FUNDAMENTAL, DETECCION ACUSTICA Y ASTRONOMIA MULTI-MENSAJERO CON TELESCOPIOS DE NEUTRINOS EN LA UPV/ info:eu-repo/grantAgreement/ANR//ANR-18-IDEX-0001 / info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-096663-B-C44/ES/FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO CON TELESCOPIOS DE NEUTRINOS EN LA UGR/ info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2018%2F034 / info:eu-repo/grantAgreement/EC/H2020/713673/EU info:eu-repo/grantAgreement/ANR//ANR-15-CE31-0020/ info:eu-repo/grantAgreement/EC/H2020/739560/EU info:eu-repo/grantAgreement/ICTP//AF-13/ info:eu-repo/grantAgreement/NCN//2015%2F18%2FE%2FST2%2F00758 / info:eu-repo/grantAgreement/Fundació Bancària Caixa d'Estalvis i Pensions de Barcelona//LCF%2FBQ%2FIN17%2F11620019/ info:eu-repo/grantAgreement/MIUR//NAT-NET 2017W4HA7S/ info:eu-repo/grantAgreement/SRNSF//FR-18-1268/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//GRISOLIAP%2F2018%2F119//AYUDA SANTIAGO GRISOLIA PROYECTO: ACUSTICA EN DETECTORES DE PARTICULAS/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//CIDEGENT%2F2019%2F043//AYUDA CONTRATACION CIDEGENT INVESTIGADORES DE EXCELENCIA-ARDID RAMIREZ, JOAN/ info:eu-repo/grantAgreement/GENERALITAT VALENCIANA//CIDEGENT%2F2019%2F043//ARTIFICIAL GENERAL INTELLIGENCE:BEYOND DEEP LEARNING/ https://doi.org/10.1140/epjc/s10052-021-09187-5 10.1093/acprof:oso/9780198508717.001.0001 10.1007/978-3-319-21846-5_109 10.1103/PhysRevD.38.448 10.1016/0168-9002(88)91097-2 10.1016/0370-2693(88)91651-6 10.1088/0954-3899/43/8/084001 10.1086/509773 10.1017/S1743921307000671 10.3847/1538-4357/aadcf7 10.1103/PhysRevD.90.045032 10.1103/PhysRevLett.111.121104 10.1103/PhysRevD.82.063007 10.1103/PhysRevD.99.063018 10.1103/PhysRevD.101.123013 10.1117/1.JATIS.5.4.046001 10.1140/epjc/s10052-014-3056-3 10.1140/epjc/s10052-015-3868-9 10.1051/0004-6361/201117810e 10.1146/annurev-nucl-102711-095006 10.1016/S0370-2693(03)00616-6 10.1142/S0217732393002567 10.1103/PhysRevD.66.013007 10.1016/j.nima.2010.06.258 10.1016/S0168-9002(03)01368-8 10.1140/epjc/s10052-020-7629-z 10.1016/j.astropartphys.2005.10.005 10.1086/305364 10.1393/ncr/i2016-10120-8 10.1140/epjc/s10052-011-1554-0 10.1140/epjc/s10052-013-2501-z http://creativecommons.org/licenses/by/4.0/ info:eu-repo/semantics/openAccess KM3NeT Core-collapse supernova Neutrinos FISICA APLICADA info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2021 ftunivpvalencia https://doi.org/10.1140/epjc/s10052-021-09187-5 2024-01-03T00:06:28Z [EN] The KM3NeT research infrastructure is under construction in the Mediterranean Sea. It consists of two water Cherenkov neutrino detectors, ARCA and ORCA, aimed at neutrino astrophysics and oscillation research, respectively. Instrumenting a large volume of sea water with 6200 optical modules comprising a total of 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to 10 MeV neutrinos from Galactic and near-Galactic core-collapse supernovae through the observation of coincident hits in photomultipliers above the background. In this paper, the sensitivity of KM3NeT to a supernova explosion is esti- mated from detailed analyses of background data from the first KM3NeT detection units and simulations of the neutrino signal. The KM3NeT observational horizon (for a 5 ¿ discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud (60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to deter- mine the arrival time of the neutrino burst with a few millisec- onds precision for sources up to 5¿8 kpc away, and detecting the peculiar signature of the standing accretion shock insta- bility if the core-collapse supernova explosion happens closer than 3¿5 kpc, depending on the progenitor mass. KM3NeT¿s capability to measure the neutrino flux spectral parameters is also presented. X The authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), ... Article in Journal/Newspaper Orca Politechnical University of Valencia: RiuNet Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) The European Physical Journal C 81 5 |