002841792 001__ 2841792
002841792 005__ 20240810042005.0
002841792 0248_ $$aoai:cds.cern.ch:2841792$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002841792 037__ $$9arXiv$$aarXiv:2211.08641$$chep-ex
002841792 037__ $$aFERMILAB-FN-1215-ND-PPD-SCD
002841792 035__ $$9arXiv$$aoai:arXiv.org:2211.08641
002841792 035__ $$9Inspire$$aoai:inspirehep.net:2182730$$d2024-08-09T18:25:25Z$$h2024-08-10T02:00:06Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002841792 035__ $$9Inspire$$a2182730
002841792 041__ $$aeng
002841792 100__ $$aHuber, Patrick$$uVirginia Tech.$$vCenter for Neutrino Physics,Physics Department,Virginia Tech,Blacksburg,VA,24061,USA
002841792 245__ $$9arXiv$$aSnowmass Neutrino Frontier Report
002841792 269__ $$c2022-11-15
002841792 300__ $$a49 p
002841792 500__ $$9arXiv$$a49 pages, contribution to: 2021 Snowmass Summer Study. Minor updates
002841792 520__ $$9arXiv$$aThis report summarizes the current status of neutrino physics and the broad and exciting future prospects identified for the Neutrino Frontier as part of the 2021 Snowmass Process.
002841792 540__ $$3preprint$$aarXiv nonexclusive-distrib 1.0$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
002841792 65017 $$2arXiv$$anucl-ex
002841792 65017 $$2SzGeCERN$$aNuclear Physics - Experiment
002841792 65017 $$2arXiv$$ahep-ph
002841792 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002841792 65017 $$2arXiv$$aastro-ph.SR
002841792 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002841792 65017 $$2arXiv$$aastro-ph.CO
002841792 65017 $$2SzGeCERN$$aAstrophysics and Astronomy
002841792 65017 $$2arXiv$$ahep-ex
002841792 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002841792 690C_ $$aCERN
002841792 690C_ $$aPREPRINT
002841792 700__ $$aScholberg, Kate$$uDuke U.$$vDepartment of Physics,Duke University,Durham,NC,27708,USA
002841792 700__ $$aWorcester, Elizabeth$$uBrookhaven$$vDepartment of Physics,Brookhaven National Laboratory,Upton,NY,11973,USA
002841792 700__ $$aAsaadi, Jonathan$$uTexas U., Arlington$$vDepartment of Physics,The University of Texas at Arlington,Arlington,TX,76019,USA
002841792 700__ $$aBalantekin, A. Baha$$uWisconsin U., Madison$$vDepartment of Physics,University of Wisconsin,Madison,Madison,WI,53706,USA
002841792 700__ $$aBowden, Nathaniel$$uLLNL, Livermore$$vLawrence Livermore National Laboratory,Livermore,CA,94550,USA
002841792 700__ $$aColoma, Pilar$$uMadrid, IFT$$vInstituto de Fisica Teorica UAM-CSIC,Campus de Cantoblanco,Madrid,28049,Spain
002841792 700__ $$aDenton, Peter B.$$uBNL, NSLS$$vHigh Energy Theory Group,Physics Department,Brookhaven National Laboratory,Upton,NY,11973,USA
002841792 700__ $$ade Gouvêa, André$$uNorthwestern U.$$vPhysics & Astronomy Department,Northwestern University,Evanston,IL,60208-3112,USA
002841792 700__ $$aFields, Laura$$uNotre Dame U.$$vDepartment of Physics and Astronomy,University of Notre Dame,IN,46556,USA
002841792 700__ $$aFriend, Megan$$uKEK, Tsukuba$$uJAERI, Tokai$$vHigh Energy Accelerator Research Organization (KEK),Tsukuba,Ibaraki,305-0801,Japan
002841792 700__ $$aGardiner, Steven$$uFermilab$$vPhysics Simulation Department,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aGiunti, Carlo$$uINFN, Turin$$vIstituto Nazionale di Fisica Nucleare (INFN),Torino,Italy
002841792 700__ $$aGruszko, Julieta$$uNorth Carolina U.$$uTUNL, Durham$$vDepartment of Physics and Astronomy,University of North Carolina at Chapel Hill,Chapel Hill,NC,27599,USA$$vTriangle Universities Nuclear Laboratory,Durham,NC,27708,USA
002841792 700__ $$aJones, Benjamin J.P.$$uTexas U., Arlington$$vDepartment of Physics,University of Texas at Arlington,Arlington,TX,76019,USA
002841792 700__ $$aKaragiorgi, Georgia$$uColumbia U.$$uColumbia U., Astron. Astrophys.$$vDepartment of Physics,Columbia University,New York,NY,10027,USA
002841792 700__ $$aKaufman, Lisa$$uSLAC$$vSLAC National Accelerator Laboratory,Menlo Park,CA,94025,USA
002841792 700__ $$aKlein, Joshua R.$$uPennsylvania U.$$vDepartment of Physics and Astronomy,University of Pennsylvania,Philadelphia,PA,19104,USA
002841792 700__ $$aKoerner, Lisa W.$$uHouston U.$$vDepartment of Physics,University of Houston,Houston,TX,77204,USA
002841792 700__ $$aKoshio, Yusuke$$uOkayama U.$$vDepartment of Physics,Okayama University,Okayama,Okayama,7000803,Japan
002841792 700__ $$aLink, Jonathan M.$$uVirginia Tech.$$vCenter for Neutrino Physics,Physics Department,Virginia Tech,Blacksburg,VA,24061,USA
002841792 700__ $$aLittlejohn, Bryce R.$$uIIT, Chicago$$vDepartment of Physics,Illinois Institute of Technology,Chicago,IL,60616,USA
002841792 700__ $$aMachado, Ana A.
002841792 700__ $$aMachado, Pedro A.N.$$uFermilab$$vTheory Division,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aMahn, Kendall$$uMichigan State U.$$vDepartment of Physics and Astronomy,Michigan State University,East Lansing,MI,48824,USA
002841792 700__ $$aMarino, Alysia D.$$uColorado U.$$vDepartment of Physics,University of Colorado Boulder,Boulder,CO,80309,USA
002841792 700__ $$aMessier, Mark D.$$uIndiana U.$$vDepartment of Physics,Indiana University,Bloomington,IN,47405,USA
002841792 700__ $$aMocioiu, Irina$$uPenn State U.$$vDepartment of Physics,Pennsylvania State University,University Park,PA,16802,USA
002841792 700__ $$aNewby, Jason$$uOak Ridge$$vPhysics Division,Oak Ridge National Laboratory,Oak Ridge,TN,37831,USA
002841792 700__ $$aO'Sullivan, Erin$$uUppsala U.$$vDepartment of Physics and Astronomy,Uppsala University,Uppsala,75120,Sweden
002841792 700__ $$aOchoa-Ricoux, Juan Pedro$$uUC, Irvine$$vDepartment of Physics and Astronomy,University of California at Irvine,Irvine,CA,92697,USA
002841792 700__ $$aOrebi Gann, Gabriel D.$$uUC, Berkeley$$uLBNL, NSD$$vDepartment of Physics,University of California at Berkeley,Berkeley,CA,94549,USA$$vNuclear Science Division,Lawrence Berkeley National Laboratory,Berkeley,CA,94549,USA
002841792 700__ $$aParno, Diana S.$$uCarnegie Mellon U.$$vDepartment of Physics,Carnegie Mellon University,Pittsburgh,PA,15217,USA
002841792 700__ $$aPastore, Saori$$uWashington U., St. Louis$$vDepartment of Physics and the McDonnell Center for the Space Sciences,Washington University in St Louis,St Louis,MO,63130,USA
002841792 700__ $$aSchmitz, David W.$$uChicago U.$$vDepartment of Physics,University of Chicago,Chicago,IL,60637,USA
002841792 700__ $$aShoemaker, Ian M.$$uVirginia Tech.$$vCenter for Neutrino Physics,Physics Department,Virginia Tech,Blacksburg,VA,24061,USA
002841792 700__ $$aSousa, Alexandre$$uCincinnati U.$$vDepartment of Physics,University of Cincinnati,Cincinnati,OH,45221,USA
002841792 700__ $$aSpitz, Joshua$$uMichigan U.$$vDepartment of Physics,University of Michigan,Ann Arbor,MI,48108,USA
002841792 700__ $$aStrauss, Raimund$$uMunich, Tech. U.$$vDepartment of Physics,Technical University Munich,Garching,85748,Germany
002841792 700__ $$aStrigari, Louis E.$$uTexas A-M$$vDepartment of Physics and Astronomy,Texas A&M University,College Station,TX,77843,USA
002841792 700__ $$aTamborra, Irene$$uBohr Inst.$$vNiels Bohr Institute,University of Copenhagen,Copenhagen,2100,Denmark
002841792 700__ $$aTanaka, Hirohisa A.
002841792 700__ $$aWang, Wei$$uZhongshan U.$$vSun Yat-Sen University,Guangzhou,China
002841792 700__ $$aYu, Jaehoon$$uTexas U., Arlington$$vDeptartment of Physics,The University of Texas at Arlington,Arlington,TX,76019,USA
002841792 700__ $$aBabu, K.S.$$uOklahoma State U.$$vDepartment of Physics,Oklahoma State University,Stillwater,OK,74078,USA
002841792 700__ $$aBernstein, Robert H.$$uFermilab$$vMuon Department,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aConley, Erin$$uDuke U.$$vDepartment of Physics,Duke University,Durham,NC,27708,USA
002841792 700__ $$aDe Roeck, Albert$$uCERN$$vEP Department,CERN,Geneva,1211,Switzerland
002841792 700__ $$aHimmel, Alexander I.$$uFermilab$$vNeutrino Division,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aJo, Jay Hyun$$uYale U.$$vDepartment of Physics,Yale University,New Haven,CT,06511,USA
002841792 700__ $$aLee, Claire$$uFermilab$$vFermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aMohayai, Tanaz A.$$uFermilab$$vNeutrino Division,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aPalladino, Kim J.$$uOxford U.$$vDepartment of Physics,University of Oxford,Oxford,OX1 3RH,UK
002841792 700__ $$aPandey, Vishvas$$uFermilab$$vNeutrino Division,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aSanchez, Mayly C.$$uFlorida State U.$$vDepartment of Physics,Florida State University,Tallahassee,FL,32306,USA
002841792 700__ $$aWong, Yvonne Y.Y.$$uNew South Wales U.$$vSchool of Physics,The University of New South Wales,Sydney,NSW,2052,Australia
002841792 700__ $$aZettlemoyer, Jacob$$uFermilab$$vNeutrino Division,Fermi National Accelerator Laboratory,Batavia,IL,60510,USA
002841792 700__ $$aZhang, Xianyi$$uLLNL, Livermore$$vLawrence Livermore National Laboratory,Livermore,CA,94536,USA
002841792 700__ $$aPocar, Andrea$$uMassachusetts U., Amherst$$vDepartment of Physics,University of Massachusetts at Amherst,Amherst,MA,01003,USA
002841792 773__ $$wC21-07-11
002841792 8564_ $$uhttps://lss.fnal.gov/archive/test-fn/1000/fermilab-fn-1215-nd-ppd-scd.pdf$$yFermilab Library Server
002841792 8564_ $$uhttps://www.slac.stanford.edu/econf/C210711/$$yeConf
002841792 8564_ $$82408751$$s65361$$uhttp://cds.cern.ch/record/2841792/files/cont_th23_dCP_nova-t2k.png$$y00001 The best-fit values of $\sinst{23}$ and $\deltacp$ to NOvA and T2K data for the normal neutrino mass ordering (top), and the inverted neutrino mass ordering (bottom)~\cite{NOvA:2021nfi}.
002841792 8564_ $$82408752$$s1354650$$uhttp://cds.cern.ch/record/2841792/files/2211.08641.pdf$$yFulltext
002841792 8564_ $$82408753$$s288837$$uhttp://cds.cern.ch/record/2841792/files/hk_sens_screenshot.png$$y00004 HK sensitivity to exclude $\sin\delta (cp) = 0$, plotted as a function of the true value of \deltacp, assuming the mass ordering is unknown. A combined fit of HK beam and atmospheric neutrinos significantly enhances the HK sensitivity to \deltacp.
002841792 8564_ $$82408754$$s101839$$uhttp://cds.cern.ch/record/2841792/files/beampowerplot_screenshot.png$$y00006 Neutrino beam power vs. energy for current and future long-baseline neutrino beams. The energy range shown here is the approximate width to half-max around the beam peak energy.
002841792 8564_ $$82408755$$s90830$$uhttp://cds.cern.ch/record/2841792/files/bubbles_atm_2019_v4_exp.png$$y00003 90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
002841792 8564_ $$82408756$$s105302$$uhttp://cds.cern.ch/record/2841792/files/bubbles_q13_2019_v4_exp.png$$y00002 90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
002841792 8564_ $$82408757$$s71058$$uhttp://cds.cern.ch/record/2841792/files/PhysicsPlansLong.png$$y00000 Summary plot of experiments indicating rough time scale and range of physics topics addressed by each. The information is provided by the collaborations. Details and references are found in Tab.~\ref{tab:experiments}.
002841792 8564_ $$82408758$$s28832$$uhttp://cds.cern.ch/record/2841792/files/guns.png$$y00005 ``Grand Unified Neutrino Spectrum" of natural neutrinos arriving at Earth (reactor neutrinos also shown). Figure from Ref.~\cite{Vitagliano:2019yzm}.
002841792 8564_ $$82409507$$s101839$$uhttp://cds.cern.ch/record/2841792/files/w6_beampowerplot_screenshot.png$$y00006 Neutrino beam power vs. energy for current and future long-baseline neutrino beams. The energy range shown here is the approximate width to half-max around the beam peak energy.
002841792 8564_ $$82409508$$s288837$$uhttp://cds.cern.ch/record/2841792/files/w4_hk_sens_screenshot.png$$y00004 HK sensitivity to exclude $\sin\delta (cp) = 0$, plotted as a function of the true value of \deltacp, assuming the mass ordering is unknown. A combined fit of HK beam and atmospheric neutrinos significantly enhances the HK sensitivity to \deltacp.
002841792 8564_ $$82409509$$s90830$$uhttp://cds.cern.ch/record/2841792/files/w3_bubbles_atm_2019_v4_exp.png$$y00003 90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
002841792 8564_ $$82409510$$s65361$$uhttp://cds.cern.ch/record/2841792/files/w1_cont_th23_dCP_nova-t2k.png$$y00001 The best-fit values of $\sinst{23}$ and $\deltacp$ to NOvA and T2K data for the normal neutrino mass ordering (top), and the inverted neutrino mass ordering (bottom)~\cite{NOvA:2021nfi}.
002841792 8564_ $$82409511$$s105302$$uhttp://cds.cern.ch/record/2841792/files/w2_bubbles_q13_2019_v4_exp.png$$y00002 90\% confidence intervals for $\sinstt{13} - \deltacp$ (left), and $\sin^2{23} - \dm{32}$ (right) after a range of exposures in kt-MW-years, for a projected measurement with assumed true parameter values near the current global best fit. Yellow regions indicate recent global fits from NuFIT 4.0.
002841792 8564_ $$82409512$$s70260$$uhttp://cds.cern.ch/record/2841792/files/w0_PhysicsPlansLong.png$$y00000 Summary plot of experiments indicating rough time scale and range of physics topics addressed by each. The information is provided by the collaborations. Details and references are found in Tab.~\ref{tab:experiments}.
002841792 8564_ $$82409513$$s28832$$uhttp://cds.cern.ch/record/2841792/files/w5_guns.png$$y00005 ``Grand Unified Neutrino Spectrum" of natural neutrinos arriving at Earth (reactor neutrinos also shown). Figure from Ref.~\cite{Vitagliano:2019yzm}.
002841792 8564_ $$82423348$$s1474710$$uhttp://cds.cern.ch/record/2841792/files/a3f285f46757fbcb9171c127e4040508.pdf$$yFulltext
002841792 960__ $$a11
002841792 962__ $$b2722743$$k$$nseattle20210711
002841792 980__ $$aConferencePaper
002841792 980__ $$aPREPRINT