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Long-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration

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cam.issuedOnline2020-10-22
dc.contributor.authorAbi, B
dc.contributor.authorAcciarri, R
dc.contributor.authorAcero, MA
dc.contributor.authorAdamov, G
dc.contributor.authorAdams, D
dc.contributor.authorAdinolfi, M
dc.contributor.authorAhmad, Z
dc.contributor.authorAhmed, J
dc.contributor.authorAlion, T
dc.contributor.authorMonsalve, SA
dc.contributor.authorAlt, C
dc.contributor.authorAnderson, J
dc.contributor.authorAndreopoulos, C
dc.contributor.authorAndrews, MP
dc.contributor.authorAndrianala, F
dc.contributor.authorAndringa, S
dc.contributor.authorAnkowski, A
dc.contributor.authorAntonova, M
dc.contributor.authorAntusch, S
dc.contributor.authorAranda-Fernandez, A
dc.contributor.authorAriga, A
dc.contributor.authorArnold, LO
dc.contributor.authorArroyave, MA
dc.contributor.authorAsaadi, J
dc.contributor.authorAurisano, A
dc.contributor.authorAushev, V
dc.contributor.authorAutiero, D
dc.contributor.authorAzfar, F
dc.contributor.authorBack, H
dc.contributor.authorBack, JJ
dc.contributor.authorBackhouse, C
dc.contributor.authorBaesso, P
dc.contributor.authorBagby, L
dc.contributor.authorBajou, R
dc.contributor.authorBalasubramanian, S
dc.contributor.authorBaldi, P
dc.contributor.authorBambah, B
dc.contributor.authorBarao, F
dc.contributor.authorBarenboim, G
dc.contributor.authorBarker, GJ
dc.contributor.authorBarkhouse, W
dc.contributor.authorBarnes, C
dc.contributor.authorBarr, G
dc.contributor.authorMonarca, JB
dc.contributor.authorBarros, N
dc.contributor.authorBarrow, JL
dc.contributor.authorBashyal, A
dc.contributor.authorBasque, V
dc.contributor.authorBay, F
dc.contributor.authorAlba, JLB
dc.contributor.authorBeacom, JF
dc.contributor.authorBechetoille, E
dc.contributor.authorBehera, B
dc.contributor.authorBellantoni, L
dc.contributor.authorBellettini, G
dc.contributor.authorBellini, V
dc.contributor.authorBeltramello, O
dc.contributor.authorBelver, D
dc.contributor.authorBenekos, N
dc.contributor.authorNeves, FB
dc.contributor.authorBerger, J
dc.contributor.authorBerkman, S
dc.contributor.authorBernardini, P
dc.contributor.authorBerner, RM
dc.contributor.authorBerns, H
dc.contributor.authorBertolucci, S
dc.contributor.authorBetancourt, M
dc.contributor.authorBezawada, Y
dc.contributor.authorBhattacharjee, M
dc.contributor.authorBhuyan, B
dc.contributor.authorBiagi, S
dc.contributor.authorBian, J
dc.contributor.authorBiassoni, M
dc.contributor.authorBiery, K
dc.contributor.authorBilki, B
dc.contributor.authorBishai, M
dc.contributor.authorBitadze, A
dc.contributor.authorBlake, A
dc.contributor.authorSiffert, BB
dc.contributor.authorBlaszczyk, FDM
dc.contributor.authorBlazey, GC
dc.contributor.authorBlucher, E
dc.contributor.authorBoissevain, J
dc.contributor.authorBolognesi, S
dc.contributor.authorBolton, T
dc.contributor.authorBonesini, M
dc.contributor.authorBongrand, M
dc.contributor.authorBonini, F
dc.contributor.authorBooth, A
dc.contributor.authorBooth, C
dc.contributor.authorBordoni, S
dc.contributor.authorBorkum, A
dc.contributor.authorBoschi, T
dc.contributor.authorBostan, N
dc.contributor.authorBour, P
dc.contributor.authorBoyd, SB
dc.contributor.authorBoyden, D
dc.contributor.authorBracinik, J
dc.contributor.authorBraga, D
dc.contributor.authorBrailsford, D
dc.date.accessioned2021-10-22T15:51:25Z
dc.date.available2021-10-22T15:51:25Z
dc.date.issued2020
dc.date.submitted2020-06-02
dc.date.updated2021-10-22T15:51:23Z
dc.description.abstractThe 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 $\delta_{\mathrm{CP}}$ 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 $\delta_{\mathrm{CP}}$ 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 $\sin^{2} 2\theta_{13}$ to current reactor experiments.
dc.identifier.arxiv2006.16043
dc.identifier.doi10.17863/CAM.77221
dc.identifier.eissn1434-6052
dc.identifier.issn1434-6044
dc.identifier.others10052-020-08456-z
dc.identifier.other8456
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/329776
dc.languageen
dc.language.isoeng
dc.publisherSpringer Science and Business Media LLC
dc.publisher.urlhttp://dx.doi.org/10.1140/epjc/s10052-020-08456-z
dc.subjecthep-ex
dc.subjecthep-ex
dc.subjecthep-ph
dc.titleLong-baseline neutrino oscillation physics potential of the DUNE experiment: DUNE Collaboration
dc.typeArticle
dcterms.dateAccepted2020-09-10
prism.issueIdentifier10
prism.publicationNameEuropean Physical Journal C
prism.volume80
rioxxterms.licenseref.urihttp://creativecommons.org/licenses/by/4.0/
rioxxterms.versionVoR
rioxxterms.versionofrecord10.1140/epjc/s10052-020-08456-z

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