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dc.contributor.authorAiello, Sebastiano
dc.contributor.authorAlbert, Arthur
dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAly, Zineb
dc.contributor.authorAmbrosone, Antonio
dc.contributor.authorAmeli, Fabrizio
dc.contributor.authorAndré, Michel
dc.contributor.authorAndroulakis, Giorgos
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnguita, M.
dc.contributor.authorAnton, Gisela
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorArdid Ramírez, Joan Salvador
dc.contributor.authorAublin, J.
dc.contributor.authorBagatelas, Christos
dc.contributor.authorBendahman, Meriem
dc.contributor.authorBenfenati, Fabio
dc.contributor.authorBertin, Vincent
dc.contributor.authorBissinger, Matthias
dc.contributor.authorBou-Cabo, M.
dc.contributor.authorBoumaaza, Jihad
dc.contributor.authorBouwhuis, M.C.
dc.contributor.authorPuricelli, Stefano
dc.contributor.authorCherubini, Silvio
dc.contributor.authorFermani, P.
dc.contributor.authorHuang, Feng
dc.contributor.authorMarkou, Christos
dc.contributor.authorMartini, Antonio
dc.contributor.authorMarzaioli, Fabio
dc.contributor.authorMiele, Gennaro
dc.contributor.authorMigliozzi, Pasquale
dc.contributor.authorMorganti, Michele
dc.contributor.authorPellegrino, Carlo
dc.contributor.authorPestel, Valentin
dc.contributor.authorPiatelli, P.
dc.contributor.authorPisanti, Ofelia
dc.contributor.authorRomanov, Artur
dc.contributor.authorSantangelo, Andrea
dc.contributor.authorStavropoulos, Dimitris
dc.contributor.authorTingay, S. J.
dc.contributor.authorTzamariudaki, Ekaterini
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2024-02-27T14:59:58Z
dc.date.available2024-02-27T14:59:58Z
dc.date.issued2021-05
dc.identifier.citationAiello, S. [et al.]. The KM3NeT potential for the next core-collapse supernova observation with neutrinos. "European physical journal C", Maig 2021, vol. 81, núm. 5, article 445.
dc.identifier.issn1434-6044
dc.identifier.otherhttps://epjc.epj.org/articles/epjc/abs/2021/05/10052_2021_Article_9187/10052_2021_Article_9187.html
dc.identifier.urihttp://hdl.handle.net/2117/403318
dc.description.abstractThe 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 corecollapse 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 s 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 determine the arrival time of the neutrino burstwith a fewmilliseconds 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.
dc.description.sponsorshipThe 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 Européenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Île-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’Università 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, Innovación, Investigación y Universidades (MCIU): Programa Estatal de Generación 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 Andalucía (ref. SOMM17/6104/UGR), Generalitat Valenciana: Grisolía (ref. GRISOLIA/2018/119) and GenT (ref. CIDEGENT/2018/034 and CIDEGENT/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’s Horizon 2020 research and innovation program under Grant agreement no 739560.
dc.language.isoeng
dc.publisherSpringer
dc.rightsAttribution 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshNeutrinos
dc.titleThe KM3NeT potential for the next core-collapse supernova observation with neutrinos
dc.typeArticle
dc.subject.lemacNeutrins
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1140/epjc/s10052-021-09187-5
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://link.springer.com/article/10.1140/epjc/s10052-021-09187-5
dc.rights.accessOpen Access
local.identifier.drac38178353
dc.description.versionPostprint (published version)
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/739560/EU/INFRADEV/KM3NeT
local.citation.authorAiello, S.; Albert, A.; Alves, S.; Zineb, A.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, G.; Ardid, M.; Ardid, J.; Aublin, J.; Bagatelas, C.; Bendahman, M.; Benfenati, F.; Bertin, V.; Bissinger, M.; Bou-Cabo, M.; Boumaaza, J.; Bouwhuis, M.; Puricelli, S.; Cherubini, S.; Fermani, P.; Huang, F.; Markou, C.; Martini, A.; Marzaioli, F.; Miele, G.; Migliozzi, P.; Morganti, M.; Pellegrino, C.; Pestel, V.; Piatelli, P.; Pisanti, O.; Romanov, A.; Santangelo, A.; Stavropoulos, D.; Tingay, S.; Tzamariudaki, E.
local.citation.publicationNameEuropean physical journal C
local.citation.volume81
local.citation.number5, article 445
dc.description.authorshipArticle signat per 246 autors/es: S. Aiello, A. Albert, S. Alves Garre, Z. Aly, A. Ambrosone, F. Ameli, M. Andre, G. Androulakis, M. Anghinolfi, M. Anguita, G. Anton, M. Ardid, S. Ardid, J. Aublin, C. Bagatelas, B. Baret, S. Basegmez du Pree, M. Bendahman, F. Benfenati, E. Berbee, A. M. van den Berg, V. Bertin, S. Biagi, M. Bissinger, M. Boettcher, M. Bou Cabo, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, H. Brânzaş, R. Bruijn, J. Brunner, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, A. Capone, V. Carretero, P. Castaldi, S. Celli, M. Chabab, N. Chau, A. Chen, S. Cherubini, V. Chiarella, T. Chiarusi, M. Circella, R. Cocimano, J. A. B. Coelho, A. Coleiro, M. Colomer Molla, R. Coniglione, P. Coyle, A. Creusot, G. Cuttone, R. Dallier, B. De Martino, M. De Palma, M. Di Marino, I. Di Palma, A. F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, M. Dörr, D. Drouhin, T. Eberl, A. Eddyamoui, T. van Eeden, D. van Eijk, I. El Bojaddaini, D. Elsaesser, A. Enzenhöfer, V. Espinosa, P. Fermani, G. Ferrara, M. D. Filipović, F. Filippini, L. A. Fusco, O. Gabella, T. Gal, A. Garcia Soto, F. Garufi, Y. Gatelet, N. Geißelbrecht, L. Gialanella, E. Giorgio, S. R. Gozzini, R. Gracia, K. Graf, D. Grasso, G. Grella, D. Guderian, C. Guidi, J. Haefner, H. Hamdaoui, H. van Haren, A. Heijboer, A. Hekalo, L. Hennig, J. J. Hernández-Rey, J. Hofestädt, F. Huang, W. Idrissi Ibnsalih, G. Illuminati, C. W. James, M. de Jong, P. de Jong, B. J. Jung, M. Kadler, P. Kalaczyński, O. Kalekin, U. F. Katz, N. R. Khan Chowdhury, G. Kistauri, F. van der Knaap, P. Kooijman, A. Kouchner, M. Kreter, V. Kulikovskiy, R. Lahmann, M. Lamoureux, G. Larosa, R. Le Breton, S. Le Stum, O. Leonardi, F. Leone, E. Leonora, N. Lessing, G. Levi, M. Lincetto, M. Lindsey Clark, T. Lipreau, F. Longhitano, D. Lopez-Coto, L. Maderer, J. Mańczak, K. Mannheim, A. Margiotta, A. Marinelli, C. Markou, L. Martin, J. A. Martínez-Mora, A. Martini, F. Marzaioli, S. Mastroianni, S. Mazzou, K. W. Melis, G. Miele, P. Migliozzi, E. Migneco, P. Mijakowski, L. S. Miranda, C. M. Mollo, M. Morganti, M. Moser, A. Moussa, R. Muller, M. Musumeci, L. Nauta, S. Navas, C. A. Nicolau, B. Ó Fearraigh, M. O’Sullivan, M. Organokov, A. Orlando, J. Palacios González, G. Papalashvili, R. Papaleo, G. Passaro, C. Pastore, A. M. Păun, G. E. Păvălaş, C. Pellegrino, M. Perrin-Terrin, V. Pestel, P. Piattelli, C. Pieterse, K. Pikounis, O. Pisanti, C. Poirè, V. Popa, T. Pradier, G. Pühlhofer, S. Pulvirenti, O. Rabyang, F. Raffaelli, N. Randazzo, S. Razzaque, D. Real, S. Reck, G. Riccobene, S. Rivoire, A. Romanov, A. Rovelli, F. Salesa Greus, D. F. E. Samtleben, A. Sánchez Losa, M. Sanguineti, A. Santangelo, D. Santonocito, P. Sapienza, J. Schnabel, M. F. Schneider, J. Schumann, H. M. Schutte, J. Seneca, I. Sgura, R. Shanidze, A. Sharma, F. Simeone, A. Sinopoulou, B. Spisso, M. Spurio, D. Stavropoulos, S. M. Stellacci, M. Taiuti, Y. Tayalati, E. Tenllado, T. Thakore, H. Thiersen, S. Tingay, V. Tsourapis, E. Tzamariudaki, D. Tzanetatos, T. Unbehaun, V. Van Elewyck, G. Vannoye, G. Vasileiadis, F. Versari, S. Viola, D. Vivolo, G. de Wasseige, J. Wilms, R. Wojaczyński, E. de Wolf, S. Zavatarelli, A. Zegarelli, D. Zito, J. D. Zornoza, J. Zúñiga & N. Zywucka


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