First searches for dark matter with the KM3NeT neutrino telescopes
[EN] Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, an excess of neutrinos is searched for in nearby dark mat...
| Autores: | , , , , , , , , , , , , , , , |
|---|---|
| Formato: | artículo |
| Fecha de publicación: | 2025 |
| País: | España |
| Recursos: | Universitat Politècnica de València (UPV) |
| Repositorio: | RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia |
| Idioma: | inglés |
| OAI Identifier: | oai:dnet:riunet______::bb8312306cba9bacdc1700152e8436ac |
| Acesso em linha: | https://riunet.upv.es/handle/10251/235529 |
| Access Level: | acceso abierto |
| Palavra-chave: | Dark matter detectors Neutrino astronomy Neutrino detectors |
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First searches for dark matter with the KM3NeT neutrino telescopes |
| title |
First searches for dark matter with the KM3NeT neutrino telescopes |
| spellingShingle |
First searches for dark matter with the KM3NeT neutrino telescopes Aiello, S. Dark matter detectors Neutrino astronomy Neutrino detectors |
| title_short |
First searches for dark matter with the KM3NeT neutrino telescopes |
| title_full |
First searches for dark matter with the KM3NeT neutrino telescopes |
| title_fullStr |
First searches for dark matter with the KM3NeT neutrino telescopes |
| title_full_unstemmed |
First searches for dark matter with the KM3NeT neutrino telescopes |
| title_sort |
First searches for dark matter with the KM3NeT neutrino telescopes |
| dc.creator.none.fl_str_mv |
Aiello, S. Albert, A. Alhebsi, A.R. Alshamsi, M. Garre, S. Alves Ambrosone, A. Ameli, F. Andre, M. Aphecetche, L. Aublin, J. Badaracco, F. Bailly-Salins, L. Ardid, Miguel|||0000-0002-3199-594X Ardid, S.|||0000-0003-4821-6655 García-Méndez, Juan|||0000-0002-1580-0647 C.A.~Quiroz-Rangel|||0009-0002-3446-8747 |
| author |
Aiello, S. |
| author_facet |
Aiello, S. Albert, A. Alhebsi, A.R. Alshamsi, M. Garre, S. Alves Ambrosone, A. Ameli, F. Andre, M. Aphecetche, L. Aublin, J. Badaracco, F. Bailly-Salins, L. Ardid, Miguel|||0000-0002-3199-594X Ardid, S.|||0000-0003-4821-6655 García-Méndez, Juan|||0000-0002-1580-0647 C.A.~Quiroz-Rangel|||0009-0002-3446-8747 |
| author_role |
author |
| author2 |
Albert, A. Alhebsi, A.R. Alshamsi, M. Garre, S. Alves Ambrosone, A. Ameli, F. Andre, M. Aphecetche, L. Aublin, J. Badaracco, F. Bailly-Salins, L. Ardid, Miguel|||0000-0002-3199-594X Ardid, S.|||0000-0003-4821-6655 García-Méndez, Juan|||0000-0002-1580-0647 C.A.~Quiroz-Rangel|||0009-0002-3446-8747 |
| author2_role |
author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Departamento de Física Aplicada Escuela Técnica Superior de Ingeniería Aeroespacial y Diseño Industrial Escuela Politécnica Superior de Gandia Instituto de Investigación para la Gestión Integrada de Zonas Costeras European Commission GENERALITAT VALENCIANA AGENCIA ESTATAL DE INVESTIGACION Agencia Estatal de Investigación Ministerio de Ciencia e Innovación Slovak Research and Development Agency Shota Rustaveli National Science Foundation Khalifa University of Science, Technology and Research Ministero dell'Istruzione, dell'Università e della Ricerca Repositorio Institucional de la Universitat Politècnica de València Riunet |
| dc.subject.none.fl_str_mv |
Dark matter detectors Neutrino astronomy Neutrino detectors |
| topic |
Dark matter detectors Neutrino astronomy Neutrino detectors |
| description |
[EN] Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, an excess of neutrinos is searched for in nearby dark matter reservoirs, such as the Sun and the Galactic Centre, which could potentially produce a sizeable flux of Standard Model particles. The KM3NeT infrastructure, currently under construction, comprises the ARCA and ORCA undersea ¿erenkov neutrino detectors located at two different sites in the Mediterranean Sea, offshore of Italy and France, respectively. The two detector configurations are optimised for the detection of neutrinos of different energies, enabling the search for dark matter particles with masses ranging from a few GeV/c2 to hundreds of TeV/c2. In this work, searches for dark matter annihilations in the Galactic Centre and the Sun with data samples taken with the first configurations of both detectors are presented. No significant excess over the expected background was found in either of the two analyses. Limits on the velocity-averaged self-annihilation cross section of dark matter particles are computed for five different primary annihilation channels in the Galactic Centre. For the Sun, limits on the spin-dependent and spin-independent scattering cross sections of dark matter with nucleons are given for three annihilation channels. |
| publishDate |
2025 |
| dc.date.none.fl_str_mv |
2025 2025-03-01 |
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journal article http://purl.org/coar/resource_type/c_6501 VoR http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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info:eu-repo/semantics/article |
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article |
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https://riunet.upv.es/handle/10251/235529 |
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https://riunet.upv.es/handle/10251/235529 |
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Inglés eng |
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Inglés |
| language |
eng |
| dc.relation.none.fl_str_mv |
Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PDC2023-145913-I00 ADQUISICION INTEGRADA EN RED Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PID2021-124591NB-C41 ELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTIMENSAJERO EN EL IFIC Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PID2021-124591NB-C42 TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UPV Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023 PID2021-124591NB-C43 TELESCOPIOS DE NEUTRINOS PARA FISICA FUNDAMENTAL Y ASTRONOMIA MULTI-MENSAJERO EN LA UGR Agence Nationale de la Recherche, Francia https://doi.org/10.13039/501100001665 ANR-10-LABX-0023 Universe: observation, modeling, transfer Agence Nationale de la Recherche, Francia https://doi.org/10.13039/501100001665 ANR-15-CE31-0020 Demonstration of Ability to Establish the Mass Ordering of Neutrinos in the Sea Agence Nationale de la Recherche, Francia https://doi.org/10.13039/501100001665 ANR-18-IDEX-0001 Université de Paris European Commission https://doi.org/10.13039/501100000780 H2020 101008324 Infrastructures for Nuclear Astrophysics European Commission https://doi.org/10.13039/501100000780 HE 101079679 Towards full implementation of the KM3NeT Research Infrastructure European Commission https://doi.org/10.13039/501100000780 HE 101142396 Multi-messenger Studies of Extragalactic Super-colliders GV INNOV.UNI.CIENCIA GV INNOV.UNI.CIENCIA ASFAE%2F2022%2F014 Telescopios submarinos de neutrinos: nuevas perspectivas GENERALITAT VALENCIANA GENERALITAT VALENCIANA CIDEGENT%2F2019%2F043 ARTIFICIAL GENERAL INTELLIGENCE:BEYOND DEEP LEARNING GENERALITAT VALENCIANA GENERALITAT VALENCIANA ESGENT%2F2024%2F24 ARTIFICIAL GENERAL INTELLIGENCE: BEYOND DEEP LEARNING- ESGENT Slovak Research and Development Agency SRDA APVV-22-0413 European Commission https://doi.org/10.13039/501100000780 MSC%2F101025085 Generalitat Valenciana https://doi.org/10.13039/501100003359 CIDEGENT%2F2020%2F049 Generalitat Valenciana https://doi.org/10.13039/501100003359 CIDEGENT%2F2018%2F034 Generalitat Valenciana https://doi.org/10.13039/501100003359 CIDEGENT%2F2021%2F23 Generalitat Valenciana https://doi.org/10.13039/501100003359 CIDEIG%2F2023%2F20 Generalitat Valenciana https://doi.org/10.13039/501100003359 CIPROM%2F2023%2F51 Generalitat Valenciana https://doi.org/10.13039/501100003359 GRISOLIAP%2F2021%2F192 Ministero dell'Istruzione dell'Università e della Ricerca, Italia https://doi.org/10.13039/501100003407 PANTHEON 2022E2J4RK Ministero dell'Istruzione dell'Università e della Ricerca, Italia https://doi.org/10.13039/501100003407 PACK-PIR01 00021 Ministero dell'Istruzione dell'Università e della Ricerca, Italia https://doi.org/10.13039/501100003407 CIR01 00021 Shota Rustaveli National Science Foundation https://doi.org/10.13039/501100004801 FR-22-13708 Agencia Estatal de Investigación http://dx.doi.org/10.13039/501100011033 CNS2023-144099 Ministerio de Ciencia e Innovación http://dx.doi.org/10.13039/501100004837 ASFAE%2F2022%2F023 KU KU ESIG-2023-008 KU KU RIG-2023-070 |
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First searches for dark matter with the KM3NeT neutrino telescopesAiello, S.Albert, A.Alhebsi, A.R.Alshamsi, M.Garre, S. AlvesAmbrosone, A.Ameli, F.Andre, M.Aphecetche, L.Aublin, J.Badaracco, F.Bailly-Salins, L.Ardid, Miguel|||0000-0002-3199-594XArdid, S.|||0000-0003-4821-6655García-Méndez, Juan|||0000-0002-1580-0647C.A.~Quiroz-Rangel|||0009-0002-3446-8747Dark matter detectorsNeutrino astronomyNeutrino detectors[EN] Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, an excess of neutrinos is searched for in nearby dark matter reservoirs, such as the Sun and the Galactic Centre, which could potentially produce a sizeable flux of Standard Model particles. The KM3NeT infrastructure, currently under construction, comprises the ARCA and ORCA undersea ¿erenkov neutrino detectors located at two different sites in the Mediterranean Sea, offshore of Italy and France, respectively. The two detector configurations are optimised for the detection of neutrinos of different energies, enabling the search for dark matter particles with masses ranging from a few GeV/c2 to hundreds of TeV/c2. In this work, searches for dark matter annihilations in the Galactic Centre and the Sun with data samples taken with the first configurations of both detectors are presented. No significant excess over the expected background was found in either of the two analyses. Limits on the velocity-averaged self-annihilation cross section of dark matter particles are computed for five different primary annihilation channels in the Galactic Centre. For the Sun, limits on the spin-dependent and spin-independent scattering cross sections of dark matter with nucleons are given for three annihilation channels.The authors acknowledge the financial support of: KM3NeT-INFRADEV2 project, funded by the European Union Horizon Europe Research and Innovation Programme under grant agreement No 101079679; Funds for Scientific Research (FRS-FNRS), Francqui foundation, BAEF foundation; Czech Science Foundation (GACR 24-12702S); 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), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Paris Ile-de-France Region, Normandy Region (Alpha, Blue-waves and Neptune), France, For the CPER The Provence-Alpes-Cote d'Azur Delegation for Research and Innovation (DRARI), the Provence-Alpes-Cote d'Azur region, the Bouches-du-Rhone Departmental Council, the Metropolis of Aix-Marseille Provence and the City of Marseille through the CPER 2021-2027 NEUMED project, The CNRS Institut National de Physique Nucleaire et de Physique des Particules (IN2P3); Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR-22-13708), Georgia; This work is part of the MuSES project which has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 Research and Innovation Programme (grant agreement No 101142396). The General Secretariat of Research and Innovation (GSRI), Greece; Istituto Nazionale di Fisica Nucleare (INFN) and Ministero dell'Universita 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; IDMAR project Po-Fesr Sicilian Region az. 1.5.1; A. De Benedittis, W. Idrissi Ibnsalih, M. Bendahman, A. Nayerhoda, G. Papalashvili, I. C. Rea, A. Simonelli have been supported by the Italian Ministero dell'Universita e della Ricerca (MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre 2019); KM3NeT4RR MUR Project National Recovery and Resilience Plan (NRRP), Mission 4 Component 2 Investment 3.1, Funded by the European Union - NextGenerationEU,CUP I57G21000040001, Concession Decree MUR No. n. Prot. 123 del 21/06/2022; 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; Ministry of Research, Innovation and Digitalisation, 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 and PDC2023-145913-I00 funded by MCIN/AEI/10.13039/501100011033 and by "ERDF A way of making Europe", for ASFAE/2022/014 and ASFAE/2022 /023 with funding from the EU NextGenerationEU (PRTR-C17.I01) and Generalitat Valenciana, for Grant AST22_6.2 with funding from Consejeria de Universidad, Investigacion e Innovacion and Gobierno de Espana and European Union - NextGenerationEU, for CSIC-INFRA23013 and for CNS2023-144099, Generalitat Valenciana for CIDEGENT/2018/034, /2019/043, /2020/049, /2021/23, for CIDEIG/2023/20, for CIPROM/2023/51 and for GRISOLIAP/2021/192 and EU for MSC/101025085, Spain; Khalifa University internal grants (ESIG-2023-008 and RIG-2023-070), United Arab Emirates; The European Union's Horizon 2020 Research and Innovation Programme (ChETEC-INFRA - Project no. 101008324)IOP PublishingDepartamento de Física AplicadaEscuela Técnica Superior de Ingeniería Aeroespacial y Diseño IndustrialEscuela Politécnica Superior de GandiaInstituto de Investigación para la Gestión Integrada de Zonas CosterasEuropean CommissionGENERALITAT VALENCIANAAGENCIA ESTATAL DE INVESTIGACIONAgencia Estatal de InvestigaciónMinisterio de Ciencia e InnovaciónSlovak Research and Development AgencyShota Rustaveli National Science FoundationKhalifa University of Science, Technology and ResearchMinistero dell'Istruzione, dell'Università e della RicercaRepositorio Institucional de la Universitat Politècnica de València Riunet20252025-03-01journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://riunet.upv.es/handle/10251/235529reponame:RiuNet. 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