The KM3NeT potential for the next core-collapse supernova observation with neutrinos

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 UnivEart...

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Published in:The European Physical Journal C
Main Authors: Aiello, S., Anguita López, Mancia, Díaz García, Antonio Francisco, López Coto, Daniel, Navas Concha, Sergio, Tenllado, Enrique, KM3NeT Collaboration
Format: Article in Journal/Newspaper
Language:English
Published: Springer 2021
Subjects:
Online Access:http://hdl.handle.net/10481/70095
https://doi.org/10.1140/epjc/s10052-021-09187-5
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description 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), Ministero dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolia (ref. GRISO-LIA/2018/119) and GenT (ref. CIDEGENT/2018/034 and CIDE-GENT/2019/043) programs, La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 713673), Spain. This work has also received funding from the European Union'sHorizon 2020 research and innovation program under Grant agreement no 739560. 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 similar to 6200 optical modules comprising a total of similar to 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to similar 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 estimated 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 sigma discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud (similar to 60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to determine the arrival time of the neutrino burst with a few milliseconds precision for sources up to 5-8 kpc away, and detecting the peculiar signature of the standing accretion shock instability 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. French National Research Agency (ANR) ANR-15-CE31-0020 Centre National de la Recherche Scientifique (CNRS) Commission Europeenne, France Institut Universitaire de France (IUF), France LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001 Paris Ile-de-France Region, France Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268 German Research Foundation (DFG) Greek Ministry of Development-GSRT Greek Ministry of Development-GSRT Istituto Nazionale di Fisica Nucleare (INFN) Ministry of Education, Universities and Research (MIUR) PRIN 2017 program, Italy NAT-NET 2017W4HA7S Ministry of Higher Education Scientific Research and Professional Training, ICTP, Morocco AF-13 Netherlands Organization for Scientific Research (NWO) Netherlands Government National Science Centre, Poland 2015/18/E/ST2/00758 National Authority for Scientific Research (ANCS), Romania Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento, Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44 Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Spain Junta de Andalucia European Commission SOMM17/6104/UGR Generalitat Valenciana: Grisolia, Spain GRISO-LIA/2018/119 GenT program, Spain CIDEGENT/2018/034 CIDE-GENT/2019/043 La Caixa Foundation LCF/BQ/IN17/11620019 EU: MSC program, Spain 713673 European Commission 739560
format Article in Journal/Newspaper
author Aiello, S.
Anguita López, Mancia
Díaz García, Antonio Francisco
López Coto, Daniel
Navas Concha, Sergio
Tenllado, Enrique
KM3NeT Collaboration
spellingShingle Aiello, S.
Anguita López, Mancia
Díaz García, Antonio Francisco
López Coto, Daniel
Navas Concha, Sergio
Tenllado, Enrique
KM3NeT Collaboration
The KM3NeT potential for the next core-collapse supernova observation with neutrinos
author_facet Aiello, S.
Anguita López, Mancia
Díaz García, Antonio Francisco
López Coto, Daniel
Navas Concha, Sergio
Tenllado, Enrique
KM3NeT Collaboration
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
publishDate 2021
url http://hdl.handle.net/10481/70095
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 info:eu-repo/grantAgreement/EC/H2020/739560
Aiello, S. [et al.]. The KM3NeT potential for the next core-collapse supernova observation with neutrinos. Eur. Phys. J. C 81, 445 (2021). [https://doi.org/10.1140/epjc/s10052-021-09187-5]
http://hdl.handle.net/10481/70095
doi:10.1140/epjc/s10052-021-09187-5
op_rights Atribución 3.0 España
http://creativecommons.org/licenses/by/3.0/es/
info:eu-repo/semantics/openAccess
op_rightsnorm CC-BY
op_doi https://doi.org/10.1140/epjc/s10052-021-09187-5
container_title The European Physical Journal C
container_volume 81
container_issue 5
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spelling ftunivgranada:oai:digibug.ugr.es:10481/70095 2023-05-15T17:54:05+02:00 The KM3NeT potential for the next core-collapse supernova observation with neutrinos Aiello, S. Anguita López, Mancia Díaz García, Antonio Francisco López Coto, Daniel Navas Concha, Sergio Tenllado, Enrique KM3NeT Collaboration 2021-05-24 http://hdl.handle.net/10481/70095 https://doi.org/10.1140/epjc/s10052-021-09187-5 eng eng Springer info:eu-repo/grantAgreement/EC/H2020/739560 Aiello, S. [et al.]. The KM3NeT potential for the next core-collapse supernova observation with neutrinos. Eur. Phys. J. C 81, 445 (2021). [https://doi.org/10.1140/epjc/s10052-021-09187-5] http://hdl.handle.net/10481/70095 doi:10.1140/epjc/s10052-021-09187-5 Atribución 3.0 España http://creativecommons.org/licenses/by/3.0/es/ info:eu-repo/semantics/openAccess CC-BY info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 2021 ftunivgranada https://doi.org/10.1140/epjc/s10052-021-09187-5 2021-09-07T23:21:11Z 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), Ministero dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Junta de Andalucia (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolia (ref. GRISO-LIA/2018/119) and GenT (ref. CIDEGENT/2018/034 and CIDE-GENT/2019/043) programs, La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 713673), Spain. This work has also received funding from the European Union'sHorizon 2020 research and innovation program under Grant agreement no 739560. 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 similar to 6200 optical modules comprising a total of similar to 200,000 photomultiplier tubes, KM3NeT will achieve sensitivity to similar 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 estimated 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 sigma discovery) covers essentially the Milky-Way and for the most optimistic model, extends to the Small Magellanic Cloud (similar to 60 kpc). Detailed studies of the time profile of the neutrino signal allow assessment of the KM3NeT capability to determine the arrival time of the neutrino burst with a few milliseconds precision for sources up to 5-8 kpc away, and detecting the peculiar signature of the standing accretion shock instability 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. French National Research Agency (ANR) ANR-15-CE31-0020 Centre National de la Recherche Scientifique (CNRS) Commission Europeenne, France Institut Universitaire de France (IUF), France LabEx UnivEarthS, France ANR-10-LABX-0023 ANR-18-IDEX-0001 Paris Ile-de-France Region, France Shota Rustaveli National Science Foundation of Georgia (SRNSFG), Georgia FR-18-1268 German Research Foundation (DFG) Greek Ministry of Development-GSRT Greek Ministry of Development-GSRT Istituto Nazionale di Fisica Nucleare (INFN) Ministry of Education, Universities and Research (MIUR) PRIN 2017 program, Italy NAT-NET 2017W4HA7S Ministry of Higher Education Scientific Research and Professional Training, ICTP, Morocco AF-13 Netherlands Organization for Scientific Research (NWO) Netherlands Government National Science Centre, Poland 2015/18/E/ST2/00758 National Authority for Scientific Research (ANCS), Romania Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento, Spain PGC2018-096663-B-C41 PGC2018-096663-A-C42 PGC2018-096663-B-C43 PGC2018-096663-B-C44 Severo Ochoa Centre of Excellence and MultiDark Consolider (MCIU), Spain Junta de Andalucia European Commission SOMM17/6104/UGR Generalitat Valenciana: Grisolia, Spain GRISO-LIA/2018/119 GenT program, Spain CIDEGENT/2018/034 CIDE-GENT/2019/043 La Caixa Foundation LCF/BQ/IN17/11620019 EU: MSC program, Spain 713673 European Commission 739560 Article in Journal/Newspaper Orca DIGIBUG: Repositorio Institucional de la Universidad de Granada Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) The European Physical Journal C 81 5