Journal article
Low exposure long-baseline neutrino oscillation sensitivity of the DUNE experiment
Physical review. D, Vol.105(7), 072006
04/25/2022
DOI: 10.1103/PhysRevD.105.072006
Abstract
The Deep Underground Neutrino Experiment (DUNE) will produce world-leading neutrino oscillation measurements over the lifetime of the experiment. In this work, we explore DUNE's sensitivity to observe charge-parity violation (CPV) in the neutrino sector, and to resolve the mass ordering, for exposures of up to 100 kiloton-megawatt-calendar years (kt-MW-CY), where calendar years include an assumption of 57% accelerator uptime based on past accelerator performance at Fermilab. The analysis includes detailed uncertainties on the flux prediction, the neutrino interaction model, and detector effects. We demonstrate that DUNE will be able to unambiguously resolve the neutrino mass ordering at a 4 sigma (5 sigma) level with a 66 (100) kt-MW-CY far detector exposure, and has the ability to make strong statements at significantly shorter exposures depending on the true value of other oscillation parameters, with a median sensitivity of 3 sigma for almost all true delta(CP) values after only 24 kt-MW-CY. We also show that DUNE has the potential to make a robust measurement of CPV at a 3 sigma level with a 100 kt-MW-CY exposure for the maximally CP-violating values delta(CP) = +/-pi/2. Additionally, the dependence of DUNE's sensitivity on the exposure taken in neutrino-enhanced and antineutrino-enhanced running is discussed. An equal fraction of exposure taken in each beam mode is found to be close to optimal when considered over the entire space of interest.
Details
- Title: Subtitle
- Low exposure long-baseline neutrino oscillation sensitivity of the DUNE experiment
- Creators
- A. Abed Abud - European Organization for Nuclear ResearchB. Abi - University of OxfordR. Acciarri - Fermi National Accelerator LaboratoryM. A. Acero - University of AtlánticoM. R. Adames - Universidade Tecnológica Federal do ParanáG. Adamov - Georgian Technical UniversityD. Adams - Brookhaven National LaboratoryM. Adinolfi - University of BristolA. Aduszkiewicz - University of HoustonJ. Aguilar - Lawrence Berkeley National LaboratoryZ. Ahmad - Variable Energy Cyclotron CentreJ. Ahmed - University of WarwickB. Aimard - Université Savoie Mont BlancB. Ali-Mohammadzadeh - Istituto Nazionale di Fisica Nucleare, Sezione di CataniaT. Alion - University of SussexK. Allison - University of Colorado BoulderS Alonso Monsalve - European Organization for Nuclear ResearchM. AlRashed - Kansas State UniversityC. Alt - ETH ZurichA. Alton - Augustana UniversityP. Amedo - Universidade de Santiago de CompostelaJ. Anderson - Argonne National LaboratoryC. Andreopoulos - University of LiverpoolM. Andreotti - Istituto Nazionale di Fisica Nucleare, Sezione di FerraraM. P. Andrews - Fermi National Accelerator LaboratoryF. Andrianala - University of AntananarivoS. Andringa - LIP - Laboratory of Instrumentation and Experimental Particle PhysicsN. Anfimov - Joint Inst Nucl Res, Dzhelepov Lab Nucl Problems 6 Joliot Curie, Dubna 141980, Moscow Region, RussiaA. Ankowski - SLAC National Accelerator LaboratoryM. Antoniassi - Universidade Tecnológica Federal do ParanáM. Antonova - Instituto de Física CorpuscularA. Antoshkin - Joint Institute for Nuclear ResearchS. Antusch - University of BaselA. Aranda-Fernandez - Univ Colima, Colima, MexicoL. O. Arnold - Columbia UniversityM. A. Arroyave - EIA UniversityJ. Asaadi - The University of Texas at ArlingtonL. Asquith - University of SussexA. Aurisano - University of CincinnatiV Aushev - Taras Shevchenko National University of KyivD. Autiero - Institute of Nuclear Physics of LyonM. Ayala-Torres - Centro de Investigación y de Estudios Avanzados del Instituto Politécnico NacionalF. Azfar - University of OxfordA. Back - Indiana University BloomingtonH. Back - Indiana University BloomingtonJ. J. Back - University of WarwickC. Backhouse - University College LondonI Bagaturia - Georgian Technical UniversityL. Bagby - Fermi National Accelerator LaboratoryN. Balashov - Joint Institute for Nuclear ResearchS. Balasubramanian - Fermi National Accelerator LaboratoryP. Baldi - University of California, IrvineB. Baller - Fermi National Accelerator LaboratoryB. Bambah - University of HyderabadF. Barao - LIP - Laboratory of Instrumentation and Experimental Particle PhysicsG. Barenboim - Universitat de ValènciaG. J. Barker - University of WarwickW. Barkhouse - University of North DakotaC. Barnes - University of MichiganG. Barr - University of OxfordJ. Barranco Monarca - Univ Guanajuato, Guanajuato 37000, MexicoA. Barros - Universidade Tecnológica Federal do ParanáN. Barros - LIP - Laboratory of Instrumentation and Experimental Particle PhysicsJ. L. Barrow - Massachusetts Institute of TechnologyA. Basharina-Freshville - University College LondonA. Bashyal - Argonne National LaboratoryV Basque - University of ManchesterE. Belchior - Universidade Estadual de Campinas (UNICAMP)J. B. R. Battat - Wellesley CollegeF. Battisti - University of OxfordF. Bay - Antalya Bilim UniversityJ. L. Bazo Alba - Pontificia Univ Catolica Peru, Lima, PeruJ. F. Beacom - The Ohio State UniversityE. Bechetoille - Institut de Physique des 2 Infinis de LyonB. Behera - Colorado State UniversityL. Bellantoni - Fermi National Accelerator LaboratoryG. Bellettini - University of PisaV Bellini - University of CataniaO. Beltramello - European Organization for Nuclear ResearchN. Benekos - European Organization for Nuclear ResearchC. Benitez Montiel - Univ Nacl Asuncion, San Lorenzo, ParaguayF. Bento Neves - Lab Instrumentacao & Fis Expt Particulas, P-1649003 Lisbon, PortugalJ. Berger - Colorado State UniversityS. Berkman - Fermi National Accelerator LaboratoryP. Bernardini - Istituto Nazionale di Fisica Nucleare, Sezione di LecceR. M. Berner - University of BernS. Bertolucci - University of BolognaM Betancourt - Fermi National Accelerator LaboratoryA. Betancur Rodriguez - Univ EIA, Envigado, Antioquia, ColombiaA. Bevan - Queen Mary University of LondonY. Bezawada - University of California, DavisT. J. C. Bezerra - University of SussexA. Bhardwaj - Louisiana State UniversityV Bhatnagar - Panjab UniversityM. Bhattacharjee - Indian Institute of Technology GuwahatiS. Bhuller - University of BristolB Bhuyan - Indian Institute of Technology GuwahatiS. Biagi - Istituto Nazionale di Fisica NucleareJ. Bian - University of California, IrvineM. Biassoni - Istituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaDUNE CollaborationMatheus Hostert (Contributor) - Physics and Astronomy
- Resource Type
- Journal article
- Publication Details
- Physical review. D, Vol.105(7), 072006
- DOI
- 10.1103/PhysRevD.105.072006
- ISSN
- 2470-0010
- eISSN
- 2470-0029
- Publisher
- Amer Physical Soc
- Number of pages
- 32
- Grant note
- ST/R006709/1 / Newton Fund; UK Research & Innovation (UKRI) ST/R000271/1; ST/S000739/1; ST/S000933/1; ST/S003452/1; ST/S000909/1; ST/W003880/1; ST/W000547/1; ST/S00372X/1; ST/W000512/1; ST/S003398/1; ST/K001337/1; ST/M002837/1; ST/S000747/1; ST/S00355X/1; ST/N000277/1; ST/S003479/1; ST/R000042/1; ST/N003233/1; ST/S003533/2; ST/M00273X/1; ST/S003568/1; ST/S003630/1; ST/S003371/1; ST/P003362/1; ST/S000712/1; ST/L002752/1; 1789818 / STFC; UK Research & Innovation (UKRI); Science & Technology Facilities Council (STFC) MR/V022407/1; MR/T019530/1; MR/T041323/1 / FLF; UK Research & Innovation (UKRI)
- Language
- English
- Date published
- 04/25/2022
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984945920602771
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