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Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies

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Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies

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dc.contributor.author Aiello, S. es_ES
dc.contributor.author Albert, A es_ES
dc.contributor.author Alshamsi, M. es_ES
dc.contributor.author Alves Garre, S. es_ES
dc.contributor.author Aly, Z. es_ES
dc.contributor.author Ambrosone, A. es_ES
dc.contributor.author Ameli, F. es_ES
dc.contributor.author Andre, M. es_ES
dc.contributor.author Androutsou, E. es_ES
dc.contributor.author Anguita, M. es_ES
dc.contributor.author Aphecetche, L. es_ES
dc.contributor.author Ardid, M. es_ES
dc.contributor.author Ardid, S. es_ES
dc.contributor.author Atmani, H. es_ES
dc.contributor.author Aublin, J. es_ES
dc.date.accessioned 2024-11-06T19:19:07Z
dc.date.available 2024-11-06T19:19:07Z
dc.date.issued 2024-10 es_ES
dc.identifier.issn 0927-6505 es_ES
dc.identifier.uri http://hdl.handle.net/10251/211436
dc.description.abstract [EN] KM3NeT/ARCA is a Cherenkov neutrino telescope under construction in the Mediterranean sea, optimised for the detection of astrophysical neutrinos with energies above similar to 1 TeV. In this work, using Monte Carlo simulations including all-flavour neutrinos, the integrated and differential sensitivities for KM3NeT/ARCA are presented considering the case of a diffuse neutrino flux as well as extended and point-like neutrino sources. This analysis is applied to Starburst Galaxies demonstrating that the detector has the capability of tracing TeV neutrinos from these sources. Remarkably, after eight years, a hard power-law spectrum from the nearby Small Magellanic Cloud can be constrained. The sensitivity and discovery potential for NGC 1068 is also evaluated showing that KM3NeT/ARCA will discriminate between different astrophysical components of the measured neutrino flux after 3 years of data taking. es_ES
dc.description.sponsorship The authors gratefully acknowledge the contribution from Damiano F. G. Fiorillo and Marco Chianese for providing support regarding SBG fluxes and for fruitful discussions. The authors acknowledge the financial support of the funding agencies: Czech Science Foundation (GAČR 24-12702S); Agence Nationale de la Recherche, France (contract ANR-15-CE31- 0020), Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Île-deFrance Region, France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-22-13708), Georgia; The General Secretariat of Research and Innovation (GSRI), Greece; Istituto Nazionale di Fisica Nucleare (INFN) and Ministero dell Università e della Ricerca (MUR), through PRIN 2022 program (Grant PANTHEON 2022E2J4RK, Next Generation EU) and PON R&I program (Avviso n. 424 del 28 febbraio 2018, Progetto PACK-PIR01 00021), Italy; A. De Benedittis, R. Del Burgo, W. Idrissi Ibnsalih, A. Nayerhoda, G. Papalashvili, I. C. Rea, S. Santanastaso, A. Simonelli have been supported by the Italian Ministero dell Università e della Ricerca (MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre 2019); Ministry of Higher Education, Scientific Research and Innovation, Morocco, and the Arab Fund for Economic and Social Development, Kuwait; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2021/41/N/ST2/01177); The grant AstroCeNT: Particle Astrophysics Science and Technology Centre , carried out within the International Research Agendas programme of the Foundation for Polish Science financed by the European Union under the European Regional Development Fund; National Authority for Scientific Research (ANCS), Romania; Slovak Research and Development Agency under Contract No. APVV-22-0413; Ministry of Education, Research, Development and Youth of the Slovak Republic; MCIN for PID2021-124591NB-C41, -C42, -C43 funded by MCIN/AEI/ 10.13039/501100011033 and, as appropriate, by ERDF A way of making Europe , by the European Union or by the European Union NextGenerationEU/PRTR , Programa de Planes Complementarios I+D+I (refs. ASFAE/2022/023, ASFAE/2022/014), Programa Prometeo (PRO METEO/2020/019) and GenT (refs. CIDEGENT/2018/034, /2019/043, /2020/049. /2021/23) of the Generalitat Valenciana, Junta de Andalucía (ref. SOMM17/6104/UGR, P18-FR-5057), EU: MSC program (ref. 101025085), Programa María Zambrano (Spanish Ministry of Universities, funded by the European Union, NextGenerationEU), Spain; The European Union s Horizon 2020 Research and Innovation Programme (ChETEC-INFRA - Project no. 101008324). es_ES
dc.language Inglés es_ES
dc.publisher Elsevier es_ES
dc.relation.ispartof Astroparticle Physics es_ES
dc.rights Reconocimiento (by) es_ES
dc.subject Neutrinos es_ES
dc.subject Sensitivity es_ES
dc.subject Differential es_ES
dc.subject Galaxies es_ES
dc.subject Starburst es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1016/j.astropartphys.2024.102990 es_ES
dc.relation.projectID info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C41/ES/ELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTIMENSAJERO EN EL IFIC/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C42/ES/TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UPV/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2021-124591NB-C43/ES/TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UGR/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Universe: observation, modeling, transfer/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-15-CE31-0020/FR/Demonstration of Ability to Establish the Mass Ordering of Neutrinos in the Sea/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-18-IDEX-0001/FR/Université de Paris/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/101008324/EU/Infrastructures for Nuclear Astrophysics/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/EC/H2020/101025085/EU/Unifying Neutrino Observatories Searches/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/SRDA//APVV-22-0413/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/Junta de Andalucía//SOMM17%2F6104%2FUGR / es_ES
dc.relation.projectID info:eu-repo/grantAgreement/Junta de Andalucía//P18-FR-5057/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2018%2F034 / es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2021%2F23/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GVA//PROMETEO%2F2020%2F019/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2019%2F043/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GVA//CIDEGENT%2F2020%2F049 / es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MIUR//2022E2J4RK/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/NCN//2021%2F41%2FN%2FST2%2F01177/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/SRNSF//FR-22-13708/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/GACR//24-12702S/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//ASFAE%2F2022%2F023/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//ASFAE%2F2022%2F014/ es_ES
dc.rights.accessRights Abierto es_ES
dc.description.bibliographicCitation Aiello, S.; Albert, A.; Alshamsi, M.; Alves Garre, S.; Aly, Z.; Ambrosone, A.; Ameli, F.... (2024). Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies. Astroparticle Physics. 162. https://doi.org/10.1016/j.astropartphys.2024.102990 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1016/j.astropartphys.2024.102990 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 162 es_ES
dc.relation.pasarela S\529035 es_ES
dc.contributor.funder European Commission es_ES
dc.contributor.funder Junta de Andalucía es_ES
dc.contributor.funder Generalitat Valenciana es_ES
dc.contributor.funder National Science Centre, Polonia es_ES
dc.contributor.funder Agencia Estatal de Investigación es_ES
dc.contributor.funder European Regional Development Fund es_ES
dc.contributor.funder Grant Agency of the Czech Republic es_ES
dc.contributor.funder Ministerio de Ciencia e Innovación es_ES
dc.contributor.funder Instituto Nazionale di Fisica Nucleare es_ES
dc.contributor.funder Slovak Research and Development Agency es_ES
dc.contributor.funder Shota Rustaveli National Science Foundation es_ES
dc.contributor.funder Arab Fund for Economic and Social Development es_ES
dc.contributor.funder Netherlands Organization for Scientific Research es_ES
dc.contributor.funder National Authority for Scientific Research, Rumanía es_ES
dc.contributor.funder General Secretariat for Research and Technology, Grecia es_ES
dc.contributor.funder Ministero dell'Istruzione, dell'Università e della Ricerca es_ES
dc.contributor.funder Ministère de l'Education Nationale, de la Formation professionnelle, de l'Enseignement Supérieur et de la Recherche Scientifique, Marruecos es_ES


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