Long-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration
dc.contributor.author | Abi, B. | |
dc.contributor.author | Acciarri, R. | |
dc.contributor.author | Acero, M. A. | |
dc.contributor.author | Adamov, G. | |
dc.contributor.author | Adams, D. | |
dc.contributor.author | Adinolfi, M. | |
dc.contributor.author | Ahmad, Z. | |
dc.date.accessioned | 2024-03-13T10:32:56Z | |
dc.date.available | 2024-03-13T10:32:56Z | |
dc.date.issued | 2020 | |
dc.department | İstanbul Beykent Üniversitesi | en_US |
dc.description.abstract | The sensitivity of the Deep Underground Neutrino Experiment (DUNE) to neutrino oscillation is determined, based on a full simulation, reconstruction, and event selection of the far detector and a full simulation and parameterized analysis of the near detector. Detailed uncertainties due to the flux prediction, neutrino interaction model, and detector effects are included. DUNE will resolve the neutrino mass ordering to a precision of 5 sigma, for all delta CP values, after 2 years of running with the nominal detector design and beam configuration. It has the potential to observe charge-parity violation in the neutrino sector to a precision of 3 sigma (5 sigma) after an exposure of 5 (10) years, for 50% of all delta CP values. It will also make precise measurements of other parameters governing long-baseline neutrino oscillation, and after an exposure of 15 years will achieve a similar sensitivity to sin22 theta 13 to current reactor experiments. | en_US |
dc.description.sponsorship | Fermi Research Alliance, LLC (FRA) [DE-AC02-07CH11359]; CNPq, Brazil; FAPERJ, Brazil; FAPEG, Brazil; FAPESP, Brazil; CFI, Canada; IPP, Canada; NSERC, Canada; CERN; MSMT, Czech Republic; ERDF, European Union; H2020-EU, European Union; MSCA, European Union; CNRS/IN2P3, France; CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Spain; Fundacion La Caixa, Spain; MICINN, Spain; SERI, Switzerland; SNSF, Switzerland; TuBTAK, Turkey; Royal Society, UK; UKRI/STFC, UK; DOE, United States of America; NSF, United States of America; National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility [DE-AC02-05CH11231]; STFC [ST/S003398/1, ST/S004696/1, ST/S000747/1, ST/M000206/1, ST/S003630/1, ST/J005428/1, ST/L005573/1, ST/S000801/1, 2192017, ST/P003362/1, ST/S000798/1, ST/S000879/1, ST/S006443/1, ST/S003878/1, ST/S00372X/1, ST/M00273X/1, ST/S003568/1, ST/R000271/1, ST/S000739/1, ST/S000933/1, ST/R000077/1, ST/S003452/1, ST/M002853/1, ST/S000909/1, ST/N000668/1, 2108560, ST/M002993/1, ST/S002308/1, ST/K00090X/1, ST/F002335/1, ST/I001204/1, ST/R000042/1, ST/K006797/1, ST/N000277/1, ST/S00355X/1, ST/R006709/1, ST/M007030/1, ST/R000085/1] Funding Source: UKRI | en_US |
dc.description.sponsorship | 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; MSMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundacion La Caixa and MICINN, Spain; SERI and SNSF, Switzerland; TuBTAK, Turkey; The Royal Society and UKRI/STFC, UK; 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.doi | 10.1140/epjc/s10052-020-08456-z | |
dc.identifier.issn | 1434-6044 | |
dc.identifier.issn | 1434-6052 | |
dc.identifier.issue | 10 | en_US |
dc.identifier.scopus | 2-s2.0-85093946110 | en_US |
dc.identifier.scopusquality | Q1 | en_US |
dc.identifier.uri | https://doi.org/10.1140/epjc/s10052-020-08456-z | |
dc.identifier.uri | https://hdl.handle.net/20.500.12662/3682 | |
dc.identifier.volume | 80 | en_US |
dc.identifier.wos | WOS:000586405100002 | en_US |
dc.identifier.wosquality | Q2 | en_US |
dc.indekslendigikaynak | Web of Science | en_US |
dc.indekslendigikaynak | Scopus | en_US |
dc.language.iso | en | en_US |
dc.publisher | Springer | en_US |
dc.relation.ispartof | European Physical Journal C | en_US |
dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | en_US |
dc.rights | info:eu-repo/semantics/openAccess | en_US |
dc.title | Long-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration | en_US |
dc.type | Article | en_US |