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Long-baseline neutrino oscillation physics potential of the DUNE experiment

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Long-baseline neutrino oscillation physics potential of the DUNE experiment. / DUNE Collaboration ; Brailsford, D.; Cross, R. et al.

In: European Physical Journal C: Particles and Fields, Vol. 80, 978, 22.10.2020.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

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DUNE Collaboration, Brailsford D, Cross R, Nowak JA, Ratoff P. Long-baseline neutrino oscillation physics potential of the DUNE experiment. European Physical Journal C: Particles and Fields. 2020 Oct 22;80:978. doi: 10.1140/epjc/s10052-020-08456-z

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DUNE Collaboration ; Brailsford, D. ; Cross, R. et al. / Long-baseline neutrino oscillation physics potential of the DUNE experiment. In: European Physical Journal C: Particles and Fields. 2020 ; Vol. 80.

Bibtex

@article{d301d7a2030d465e91314a6411ce2aac,
title = "Long-baseline neutrino oscillation physics potential of the DUNE experiment",
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 hierarchy 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. ",
keywords = "hep-ex, hep-ph",
author = "{DUNE Collaboration} and B. Abi and R. Acciarri and Acero, {M. A.} and G. Adamov and D. Adams and M. Adinolfi and Z. Ahmad and J. Ahmed and T. Alion and Monsalve, {S. Alonso} and C. Alt and C. Andreopoulos and Andrews, {M. P.} and F. Andrianala and S. Andringa and A. Ankowski and M. Antonova and S. Antusch and A. Aranda-Fernandez and A. Ariga and Arnold, {L. O.} and Arroyave, {M. A.} and J. Asaadi and A. Aurisano and V. Aushev and D. Autiero and F. Azfar and H. Back and Back, {J. J.} and C. Backhouse and P. Baesso and L. Bagby and R. Bajou and S. Balasubramanian and P. Baldi and B. Bambah and F. Barao and G. Barenboim and Barker, {G. J.} and W. Barkhouse and C. Barnes and G. Barr and Monarca, {J. Barranco} and N. Barros and A. Blake and D. Brailsford and R. Cross and Nowak, {J. A.} and P. Ratoff",
year = "2020",
month = oct,
day = "22",
doi = "10.1140/epjc/s10052-020-08456-z",
language = "English",
volume = "80",
journal = "European Physical Journal C: Particles and Fields",
issn = "1434-6044",
publisher = "SPRINGER",

}

RIS

TY - JOUR

T1 - Long-baseline neutrino oscillation physics potential of the DUNE experiment

AU - DUNE Collaboration

AU - Abi, B.

AU - Acciarri, R.

AU - Acero, M. A.

AU - Adamov, G.

AU - Adams, D.

AU - Adinolfi, M.

AU - Ahmad, Z.

AU - Ahmed, J.

AU - Alion, T.

AU - Monsalve, S. Alonso

AU - Alt, C.

AU - Andreopoulos, C.

AU - Andrews, M. P.

AU - Andrianala, F.

AU - Andringa, S.

AU - Ankowski, A.

AU - Antonova, M.

AU - Antusch, S.

AU - Aranda-Fernandez, A.

AU - Ariga, A.

AU - Arnold, L. O.

AU - Arroyave, M. A.

AU - Asaadi, J.

AU - Aurisano, A.

AU - Aushev, V.

AU - Autiero, D.

AU - Azfar, F.

AU - Back, H.

AU - Back, J. J.

AU - Backhouse, C.

AU - Baesso, P.

AU - Bagby, L.

AU - Bajou, R.

AU - Balasubramanian, S.

AU - Baldi, P.

AU - Bambah, B.

AU - Barao, F.

AU - Barenboim, G.

AU - Barker, G. J.

AU - Barkhouse, W.

AU - Barnes, C.

AU - Barr, G.

AU - Monarca, J. Barranco

AU - Barros, N.

AU - Blake, A.

AU - Brailsford, D.

AU - Cross, R.

AU - Nowak, J. A.

AU - Ratoff, P.

PY - 2020/10/22

Y1 - 2020/10/22

N2 - 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 hierarchy 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.

AB - 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 hierarchy 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.

KW - hep-ex

KW - hep-ph

U2 - 10.1140/epjc/s10052-020-08456-z

DO - 10.1140/epjc/s10052-020-08456-z

M3 - Journal article

VL - 80

JO - European Physical Journal C: Particles and Fields

JF - European Physical Journal C: Particles and Fields

SN - 1434-6044

M1 - 978

ER -