Deep underground neutrino experiment (DUNE) near detector conceptual design report

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dc.contributor.authorAbud A.A.
dc.contributor.authorAbi B.
dc.contributor.authorAcciarri R.
dc.contributor.authorAcero M.A.
dc.contributor.authorAdamov G.
dc.contributor.authorAdams D.
dc.contributor.authorAdinolfi M.
dc.date.accessioned2024-03-13T10:01:14Z
dc.date.available2024-03-13T10:01:14Z
dc.date.issued2021
dc.departmentİstanbul Beykent Üniversitesien_US
dc.description.abstractThe Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment consists of a near detector, sited close to the source of the beam, and a far detector, sited along the beam at a large distance. This document, the DUNE Near Detector Conceptual Design Report (CDR), describes the design of the DUNE near detector and the science program that drives the design and technology choices. The goals and requirements underlying the design, along with projected performance are given. It serves as a starting point for a more detailed design that will be described in future documents. © 2021 by the authors. Licensee MDPI, Basel, Switzerland.en_US
dc.description.sponsorshipDE-AC02-07CH11359; National Science Foundation, NSF; U.S. Department of Energy, USDOE: DE-AC02-05CH11231; Multiple Sclerosis Center of Atlanta, MSCA; CERN; UK Research and Innovation, UKRI; Natural Sciences and Engineering Research Council of Canada, NSERC; Science and Technology Facilities Council, STFC; Royal Society; European Commission, EC; Singapore Eye Research Institute, SERI; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, SNF; Fundação de Amparo à Pesquisa do Estado de São Paulo, FAPESP; Ministerstvo Školství, Mláde?e a T?lov?chovy, MŠMT; Fundação para a Ciência e a Tecnologia, FCT; Generalitat Valenciana, GVA; Conselho Nacional de Desenvolvimento Científico e Tecnológico, CNPq; National Research Foundation of Korea, NRF; Instituto Nazionale di Fisica Nucleare, INFN; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, FAPERJ; Centre National de la Recherche Scientifique, CNRS; Ministerio de Ciencia e Innovación, MICINN; Fundação de Amparo à Pesquisa do Estado de Goiás, FAPEG; Commissariat à l'Énergie Atomique et aux Énergies Alternatives, CEA; European Regional Development Fund, ERDF; Xunta de Galicia; Agencia Estatal de Investigación, AEI; Institut National de Physique Nucléaire et de Physique des Particules, IN2P3en_US
dc.description.sponsorshipFunding: This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America.en_US
dc.description.sponsorshipFERMILAB-PUB-21-067-E-LBNF-PPD-SCD-T This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.en_US
dc.identifier.doi10.3390/instruments5040031
dc.identifier.issn2410-390X
dc.identifier.issue4en_US
dc.identifier.scopus2-s2.0-85120872170
dc.identifier.scopusqualityQ3en_US
dc.identifier.urihttps://doi.org/10.3390/instruments5040031
dc.identifier.urihttps://hdl.handle.net/20.500.12662/3067
dc.identifier.volume5en_US
dc.indekslendigikaynakScopus
dc.language.isoenen_US
dc.publisherMDPIen_US
dc.relation.ispartofInstrumentsen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectDeep Underground Neutrino Experimenten_US
dc.subjectDUNEen_US
dc.subjectNear detectoren_US
dc.subjectNeutrinoen_US
dc.subjectNeutrino oscillationsen_US
dc.titleDeep underground neutrino experiment (DUNE) near detector conceptual design reporten_US
dc.typeArticleen_US

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