Long-baseline neutrino oscillation physics potential of the DUNE experiment

B. Abi; R. Acciarri; M. A. Acero; G. Adamov; D. Adams; M. Adinolfi; Z. Ahmad; J. Ahmed; T. Alion; S Alonso Monsalve; C. Alt; J. Anderson; C. Andreopoulos; M. P. Andrews; F. Andrianala; S. Andringa; A. Ankowski; M. Antonova; A. Aranda-Fernandez; S. Antusch; A. Ariga; L. O. Arnold; M. A. Arroyave; J. Asaadi; A. Aurisano; V. Aushev; D. Autiero; F. Azfar; H. Back; J. J. Back; C. Backhouse; P. Baesso; L. Bagby; R. Bajou; S. Balasubramanian; P. Baldi; B. Bambah; F. Barao; G. Barenboim; G. J. Barker; W. Barkhouse; C. Barnes; G. Barr; J Barranco Monarca; N. Barros; J. L. Barrow; A. Bashyal; V. Basque; F. Bay; J. L. Bazo Alba; J. F. Beacom; E. Bechetoille; B. Behera; L. Bellantoni; G. Bellettini; V. Bellini; O. Beltramello; D. Belver; N. Benekos; F. Bento Neves; J. Berger; S. Berkman; P. Bernardini; R. M. Berner; H. Berns; S. Bertolucci; M. Betancourt; Y. Bezawada; M. Bhattacharjee; B. Bhuyan; S. Biagi; J. Bian; M. Biassoni; K. Biery; B. Bilki; M. Bishai; A. Bitadze; A. Blake; B. Blanco Siffert; F. D. M. Blaszczyk; G. C. Blazey; E. Blucher; J. Boissevain; S. Bolognesi; T. Bolton; M. Bonesini; M. Bongrand; F. Bonini; A. Booth; C. Booth; S. Bordoni; A. Borkum; T. Boschi; N. Bostan; P. Bour; S. B. Boyd; D. Boyden; J. Bracinik; D. Braga; D. Brailsford; DUNE Collaboration; Matheus Hostert

doi:10.1140/epjc/s10052-020-08456-z

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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

B. Abi, R. Acciarri, M. A. Acero, G. Adamov, D. Adams, M. Adinolfi, Z. Ahmad, J. Ahmed, T. Alion, S Alonso Monsalve, …

The European physical journal. C, Particles and fields, Vol.80(10), 978

10/2020

DOI: 10.1140/epjc/s10052-020-08456-z

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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.

Physical Sciences

Physics

Physics, Particles & Fields

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Title: Subtitle: Long-baseline neutrino oscillation physics potential of the DUNE experiment
Creators: B. Abi - Institute for Nuclear Research
R. Acciarri - Fermi National Accelerator Laboratory
M. A. Acero - University of Atlántico
G. Adamov - Georgian Technical University
D. Adams - Brookhaven National Laboratory
M. Adinolfi - University of Bristol
Z. Ahmad - Variable Energy Cyclotron Centre
J. Ahmed - University of Warwick
T. Alion - University of Sussex
S Alonso Monsalve - European Organization for Nuclear Research
C. Alt - ETH Zurich
J. Anderson - Argonne National Laboratory
C. Andreopoulos - University of Liverpool
M. P. Andrews - Fermi National Accelerator Laboratory
F. Andrianala - University of Antananarivo
S. Andringa - LIP - Laboratory of Instrumentation and Experimental Particle Physics
A. Ankowski - SLAC National Accelerator Laboratory
M. Antonova - Instituto de Física Corpuscular
A. Aranda-Fernandez - Univ Colima, Colima, Mexico
S. Antusch - University of Basel
A. Ariga - University of Bern
L. O. Arnold - Columbia University
M. A. Arroyave - EIA University
J. Asaadi - The University of Texas at Arlington
A. Aurisano - University of Cincinnati
V. Aushev - Kyiv Natl Univ, UA-01601 Kiev, Ukraine
D. Autiero - Institut de Physique des 2 Infinis de Lyon
F. Azfar - University of Oxford
H. Back - Pacific Northwest National Laboratory
J. J. Back - University of Warwick
C. Backhouse - University College London
P. Baesso - University of Bristol
L. Bagby - Fermi National Accelerator Laboratory
R. Bajou - Laboratoire AstroParticule et Cosmologie
S. Balasubramanian - Yale University
P. Baldi - University of California, Irvine
B. Bambah - University of Hyderabad
F. Barao - University of Lisbon
G. Barenboim - Instituto de Física Corpuscular
G. J. Barker - University of Warwick
W. Barkhouse - University of North Dakota
C. Barnes - University of Michigan
G. Barr - University of Oxford
J Barranco Monarca - Universidad de Guanajuato
N. Barros - University of Lisbon
J. L. Barrow - Fermi National Accelerator Laboratory
A. Bashyal - Oregon State University
V. Basque - University of Manchester
F. Bay - National Institute for Subatomic Physics
J. L. Bazo Alba - Pontifical Catholic University of Peru
J. F. Beacom - The Ohio State University
E. Bechetoille - Institut de Physique des 2 Infinis de Lyon
B. Behera - Colorado State University
L. Bellantoni - Fermi National Accelerator Laboratory
G. Bellettini - University of Pisa
V. Bellini - University of Catania
O. Beltramello - European Organization for Nuclear Research
D. Belver - Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas
N. Benekos - European Organization for Nuclear Research
F. Bento Neves - Lab Instrumentacao & Fis Expt Particulas, P-1649003 Lisbon, Portugal
J. Berger - University of Pittsburgh
S. Berkman - Fermi National Accelerator Laboratory
P. Bernardini - Istituto Nazionale di Fisica Nucleare, Sezione di Lecce
R. M. Berner - University of Bern
H. Berns - University of California, Davis
S. Bertolucci - University of Bologna
M. Betancourt - Fermi National Accelerator Laboratory
Y. Bezawada - University of California, Davis
M. Bhattacharjee - Indian Institute of Technology Guwahati
B. Bhuyan - Indian Institute of Technology Guwahati
S. Biagi - Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud
J. Bian - University of California, Irvine
M. Biassoni - Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca
K. Biery - Fermi National Accelerator Laboratory
B. Bilki - Beykent University
M. Bishai - Brookhaven National Laboratory
A. Bitadze - University of Manchester
A. Blake - Lancaster University
B. Blanco Siffert - Universidade Federal do Rio de Janeiro
F. D. M. Blaszczyk - Fermi National Accelerator Laboratory
G. C. Blazey - Northern Illinois University
E. Blucher - University of Chicago
J. Boissevain - Los Alamos National Laboratory
S. Bolognesi - Institut de Recherche sur les Lois Fondamentales de l'Univers
T. Bolton - Kansas State University
M. Bonesini - Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca
M. Bongrand - Grand Accélérateur National d'Ions Lourds
F. Bonini - Brookhaven National Laboratory
A. Booth - University of Sheffield
C. Booth - University of Sheffield
S. Bordoni - European Organization for Nuclear Research
A. Borkum - University of Sussex
T. Boschi - Durham University
N. Bostan - University of Iowa
P. Bour - Czech Technical University in Prague
S. B. Boyd - University of Warwick
D. Boyden - Northern Illinois University
J. Bracinik - University of Birmingham
D. Braga - Fermi National Accelerator Laboratory
D. Brailsford - Lancaster University
DUNE Collaboration
Matheus Hostert (Contributor) - Physics and Astronomy
Resource Type: Journal article
Publication Details: The European physical journal. C, Particles and fields, Vol.80(10), 978
DOI: 10.1140/epjc/s10052-020-08456-z
ISSN: 1434-6044
eISSN: 1434-6052
Publisher: Springer Nature
Number of pages: 34
Grant note: CERN FAPEG, Brazil; Fundacao de Amparo a Pesquisa do Estado do Goias (FAPEG) IPP, Canada UKRI/STFC, UK INFN, Italy; Istituto Nazionale di Fisica Nucleare (INFN) ST/S003452/1; ST/I001204/1; ST/M000206/1; ST/S003630/1; ST/J005428/1; ST/R000042/1; ST/K006797/1; ST/N000277/1; ST/M007030/1; ST/R000085/1; ST/P003362/1; ST/L005573/1; ST/S000801/1; ST/S000747/1; ST/S004696/1; ST/S003398/1; ST/M002853/1; ST/S000933/1; ST/S000739/1; ST/R000271/1; ST/S003568/1; ST/M00273X/1; ST/F002335/1; ST/K00090X/1; ST/S002308/1; ST/S00372X/1; ST/S003878/1; ST/S006443/1; ST/S000879/1; ST/S000798/1; ST/S00355X/1; 2192017; ST/S000909/1; ST/N000668/1; 2108560; ST/M002993/1; ST/R000077/1 / STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) CNRS/IN2P3, France; Centre National de la Recherche Scientifique (CNRS) FCT, Portugal; Fundacao para a Ciencia e a Tecnologia (FCT) NSF, United States of America; National Science Foundation (NSF) FAPESP, Brazil; Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)
Language: English
Date published: 10/2020
Academic Unit: Physics and Astronomy
Record Identifier: 9984945919102771

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